Monthly Notices of the Royal Astronomical Society 1998: Vol 293-304 Index

113 Pages·1998·34.4 MB·English

Monthly Notices
OF THE
Royal Astronomical
Society
VOLUME 301
1998 NOVEMBER 21-— DECEMBER 21]
(INCORPORATING ANNUAL INDEX VOLS 293-301)
The Board of Editors
PROFESSOR M. J. BARLOW, DEPARTMENT OI
PHYSICS AND ASTRONOMY, UNIVERSITY
COLLEGE LONDON
DR R. F. CARSWELL (DEPUTY MANAGING
EDITOR), INSTITUTE OF ASTRONOMY,
CAMBRIDGI
DR J. E. DREW, ASTRONOMY GROUP
BLACKETT LABORATORY, IMPERIAI
COLLEGE LONDON
PROFESSOR A. C. FABIAN FRS (MANAGING
EDITOR), INSTITUTE OF ASTRONOMY
CAMBRIDGI
PROFESSOR M. W. FEAST, DEPARTMENT OF
ASTRONOMY, UNIVERSITY OF CAPE TOWN
PROFESSOR D. R. FLOWER, DEPARTMENT OF
PHYSICS, UNIVERSITY OF DURHAM
PROFESSOR D. C. HEGGIE, DEPARTMENT OF
MATHEMATICS & STATISTICS, UNIVERSITY
OF EDINBURGH
DR D. W. HUGHES, DEPARTMENT OI!
PHYSICS, UNIVERSITY OF SHEFFIELD
PROFESSOR J. C. B. PAPALOIZOU, SCHOOL OIF
MATHEMATICAL SCIENCES, QUEEN MARY &
WESTFIELD COLLEGE LONDON
DR P. A. G. SCHEUER, CAVENDISH LABORATORY,
CAMBRIDGI
PROFESSOR M. J. WARD, DEPARTMENT OF
PHYSICS & ASTRONOMY, UNIVERSITY OF
LEICESTER
PROFESSOR S. D. M. WHITE, MAX-PLANCK
INSTITUT FUR ASTROPHYSIK, GARCHING BEI
MUNCHEN
Published for the
Royal Astronomical Society by
Blackwell Science
OXFORD LONDON EDINBURGH
BOSTON MELBOURNI
TOKYO BERLIN VIENNA

Mon. Not. R. Astron. Soc. 301 (1998)
List of key words used in the annual subject indexes
(valid from January 1998)
This list is common to Monthly Notices of the Royal nuclear reactions, nucleosynthesis, abundances
Astronomical Society, Astronomy and Astrophysics, plasmas
and The Astrophysical Journal. In order to ease the polarization
search, the key words are subdivided into broad cate- radiation mechanisms: non-thermal
gories. No more than six subcategories altogether radiation mechanisms: thermal
should be listed for a paper. radiative transfer
The subcategories in boldface containing the word relativity
‘individual’ are intended for use with specific astro- scattering
nomical objects; these should never be used alone, but shock waves
always in combination with the most common names turbulence
for the astronomical objects in question. Note that each waves
object counts as one subcategory within the allowed
limit of six. Astronomical instrumentation, methods and
The parts of the key words in italics are for reference techniques
only and should be omitted when the key words are
entered on the manuscript. atmospheric effects
balloons
instrumentation: detectors
General
instrumentation: interferometers
book reviews instrumentation: miscellaneous
editorials, notices instrumentation: photometers
errata, addenda instrumentation: polarimeters
extraterrestrial intelligence instrumentation: spectrographs
history and philosophy of astronomy methods: analytical
miscellaneous methods: data analysis
obituaries, biographies methods: laboratory
methods: miscellaneous
Physical data and processes methods: numerical
acceleration of particles methods: observational
methods: statistical
accretion, accretion discs
site testing
atomic data
space vehicles
atomic processes
techniques: image processing
black hole physics
techniques: interferometric
chaos
techniques: miscellaneous
conduction
techniques: photometric
convection
techniques: polarimetric
cosmic strings
techniques: radar astronomy
dense matter
techniques: radial velocities
diffusion
techniques: spectroscopic
elementary particles
telescopes
equation of state
gravitation
hydrodynamics Astronomical data bases
instabilities
astrodanta obasmes: imicsceallalneo us
line: formation
atlases
line: identification
catalogues
line: profiles surveys
magnetic fields
(magnetohydrodynamics) MHD
Astrometry and celestial mechanics
masers
molecular data astrometry
molecular processes celestial mechanics, stellar dynamics
© 1998 RAS
Index ke words
stars: carbon
eclipses
ephemerides stars: chemically peculiar
occultations stars: chromospheres
reference systems (stars:) circumstellar matter
time Stars: coronae
Stars: distances
The Sun stars: early-type
stars: emission-line, Be
Sun: abundances
Stars: evolution
Sun: activity
stars: flare
Sun: atmosphere
Stars: formation
Sun: chromosphere
stars: fundamental parameters (classification,
Sun: corona
colours, luminosities, masses, radii,
Sun: evolution
temperatures, etc.)
Sun: faculae, plages
Stars: general
Sun: filaments
(stars: )H ertzsprung—Russell (HR) diagram
Sun: flares
stars: horizontal branch
Sun: fundamental parameters
Stars: imaging
Sun: general
stars: individual...
Sun: granulation
Stars: interiors
Sun: infrared
Stars: kinematics
Sun: interior
stars: late-type
Sun: magnetic fields
stars: low-mass, brown dwarfs
Sun: oscillations
stars: luminosity function, mass function
Sun: particle emission
stars: magnetic fields
Sun: photosphere
stars: mass-loss
Sun: prominences
stars: neutron
Sun: radio radiation
(stars:) novae, cataclysmic variables
Sun: rotation
stars: oscillations (including pulsations)
(Sun: ) solar—terrestrial relations
stars: peculiar (except chemically peculiar)
(Sun:) solar wind
(stars:) planetary systems
(Sun:) sunspots
stars: Population II
Sun: transition region
stars: pre-main-sequence
Sun: UV radiation
(stars:) pulsars: general
Sun: X-rays, gamma-rays
(stars:) pulsars: individual:...
Stars: rotation
Solar system
Stars: Stauistics
comets: general (stars: ) subdwarts
comets: individual:... (stars: ) supergiants
Earth (stars:) supernovae: general
interplanetary medium (stars:) supernovae: individual:...
meteors, meteoroids (stars: variables: ) Cepheids
minor planets, asteroids (stars: variables: ) 6 Scuti
Moon Stars: variables: other
planets and satellites: general (stars:) white dwarts
planets and satellites: individual... stars: Wolf—Rayet
Solar system: formation
Solar system: general Interstellar medium (ISM), nebulae
ISM: abundances
Stars
ISM: atoms
stars: abundances ISM: bubbles
Stars: activity ISM: clouds
stars: AGB and post-AGB (1SM:) cosmic rays
stars: atmospheres (1SM:) dust, extinction
(stars:) binaries (including multiple): close ISM: general
(stars:) binaries: eclipsing ISM: globules
(stars:) binaries: general (1SM:) Hui regions
(stars:) binaries: spectroscopic ISM: individual...
(stars:) binaries: symbiotic (except planetary nebulae)
(stars:) binaries: visual ISM: jets and outflows
(stars:) blue stragglers ISM: kinematics and dynamics
© 1998 RAS
Index key words
ISM: magnetic fields galaxies: photometry
ISM: molecules (galaxies: )q uasars: absorption lines
(1SM:) planetary nebulae: general (galaxies: )q uasars: emission lines
(1SM:) planetary nebulae: individual:... (galaxies: )q uasars: general
(1SM:) reflection nebulae (galaxies:) quasars: individual...
ISM: structure galaxies: Seyfert
(1SM:) supernova remnants galaxies: spiral
galaxies: starburst
The Galaxy galaxies: star clusters
galaxies: statistics
Galaxy: abundances
galaxies: stellar content
Galaxy: centre
galaxies: structure
Galaxy: evolution
Galaxy: formation
Cosmology
Galaxy: fundamental parameters
Galaxy: general (cosmology: ) cosmic microwave background
(Galaxy:) globular clusters: general cosmology: miscellaneous
(Galaxy:) globular clusters: individual... cosmology: observations
Galaxy: halo cosmology: theory
Galaxy: kinematics and dynamics (cosmology: ) dark matter
(Galaxy: ) open clusters and associations: general (cosmology: ) diffuse radiation
(Galaxy: )o pen clusters and associations: individual:... (cosmology: ) distance scale
(Galaxy: ) solar neighbourhood (cosmology:) early Universe
Galaxy: stellar content (cosmology: ) gravitational lensing
Galaxy: structure (cosmology: ) large-scale structure of Universe
Galaxies Sources as a function of wavelength
galaxies: abundances gamma-rays: bursts
galaxies: active gamma-rays: observations
(galaxies:) BL Lacertae objects: general gamma-rays: theory
(galaxies:) BL Lacertae objects: individual:... infrared: galaxies
galaxies: clusters: general infrared: general
galaxies: clusters: individual:... infrared: ISM: continuum
galaxies: compact infrared: ISM: lines and bands
(galaxies:) cooling flows infrared: Solar system
galaxies: distances and redshifts infrared: stars
galaxies: elliptical and lenticular, cD radio continuum: galaxies
galaxies: evolution radio continuum: general
galaxies: formation radio continuum: ISM
galaxies: fundamental parameters radio continuum: Solar system
(classification, colours, luminosities, masses, radii, etc.) radio continuum: stars
galaxies: general radio lines: galaxies
galaxies: haloes radio lines: general
galaxies: individual... radio lines: ISM
galaxies: interactions radio lines: Solar system
(galaxies: ) intergalactic medium radio lines: stars
galaxies: ISM ultraviolet: galaxies
galaxies: irregular ultraviolet: general
galaxies: jets ultraviolet: ISM
galaxies: kinematics and dynamics ultraviolet: Solar system
(galaxies:) Local Group ultraviolet: stars
galaxies: luminosity function, mass function X-rays: bursts
(galaxies:) Magellanic Clouds X-rays: galaxies
galaxies: magnetic fields X-rays: general
galaxies: nuclei X-rays: ISM
galaxies: peculiar X-rays: stars
‘ 1998 R AS

Mon. Not. R. Astron. Soc. 293—301 (1998)
Subject index
General Observations of the SW Sextantis star UU Aquarii (Hoard D.W.., Still
M.D., Szkody P., Smith R.C., Buckley D.A.H.), 294, 689
Editorials, notices Global solutions of adiabatic accretion flows with isothermal shocks in
Editorial: submission of accepted papers in I pX/L* I px by FTP, 295, Kerr black hole geometry (Lu J.-F., Yuan F.), 295, 66
4 ASCA X-ray observations of EX Hya: spin-resolved spectroscopy
(Allan A., Hellier C., Beardmore A.), 295, 167
Errata, addenda Polarimetry of QQ Vul (Cropper M.), 295, 353
Erratum: Paramagnetic alignment of thermally rotating dust (Lazarian Radiation-driven winds from luminous accretion discs (Proga D
\.), 293, 208 Stone J.M., Drew J.E.), 295, 595
Erratum: Spiral structure in the accretion disc of the binary IP Pegasi Supersonic wind accretion in massive close binary systems: a 3D
(Steeghs D., Harlaftis E.T., Horne K.), 296, 463 SPH simulation of Cen X-3 (Lanzafame G., Belvedere G.), 295,
618
Erratum: Collapse of a radiating star with shear (Chan R.), 299, 811
Erratum: Metallicity and photospheric abundances in field K and M Multiwavelength monitoring of GRS 1915 + 105 (Bandyopadhyay R..,
dwarts (Zboril M., Byrne P.B., Rolleston W.R.J.), 301, 1104 Martini P., Gerard E., Charles P.A., Wagner R.M., Shrader C.,
Shahbaz T., Mirabel I.F.), 295, 623
Polarimetry of the eclipsing polar RX JO929.1—2404 (Buckley D.A.H.,
Ferrario L., Wickramasinghe D.T., Bailey J.A.), 295, 899
Physical data and processes
On the outburst amplitude of the soft X-ray transients (Shahbaz T..,
Kuulkers E.), 295, L1
Acceleration of particles Spiral shocks in accretion discs (Godon P., Livio M., Lubow S.), 295,
The Deutsch field gamma-ray pulsar — IJ. Application of the model Lil
(Higgins M.G., Henriksen R.N.), 295, 188 On the orbital period distribution of cataclysmic variables (Hellier C.,
Naylor T.), 295, L50
Accretion, accretion discs 3+ 1 formulation of non-ideal hydrodynamics (Peitz J., Appl S.), 296,
Polarization from magnetized accretion discs — II. The effects of 231
absorption opacity on Faraday rotation (Agol E., Blaes O., lonescu Gamma-ray bursts from internal shocks in a relativistic wind: temporal
Zanetti C.), 293, | and spectral properties (Daigne F., Mochkovitch R.), 296, 275
Nova V1425 Aquilae 1995: the early appearance of accretion Impact of small bodies on to discs around compact objects — Il
processes in an intermediate polar candidate (Retter A., Leibowitz Interaction with the disc (Landry S., Pineault S.), 296, 359
E.M., Kovo-KaritiO .), 293, 145 Discovery of the high-field polar RX J1724.0 + 4114 (Greiner J.,
White dwarf masses in magnetic cataclysmic variables: multi Schwarz R., Wenzel W.), 296, 437
temperature fits to Ginga data (Cropper M., Ramsay G., Wu K.), Erratum: Spiral structure in the accretion disc of the binary IP Pegasi
293, 222 (Steeghs D., Harlaftis E.T., Horne K.), 296, 463
Limits from rapid TeV variability of Mrk 421 (Celotti A., Fabian A.C., rhe mass of the white dwarf in the old nova BT Mon (Smith D.A.,
Dhillon V.S., Marsh T.R.), 296, 465
Rees M.J.), 293, 239
rhe biconical kiloparsec structure generated by nuclear starbursts A radiation-driven disc wind model for massive young stellar objects
(Tenorio-TagleG ., Muitoz-Tunén C.), 293, 299 (Drew J.E., Proga D., Stone J.M.), 296, L6
\ note on the conditions for SSD-ADAF transitions (Abramowicz Predicting the future of superhumps in classical nova systems (Rettet
M.A., Igumenshchev I.V., Lasota J.-P), 293, 443 A., Leibowitz E.M.), 296, L37
Stellar capture by an accretion disc (Vokrouhlicky D., Karas V.), 293, Outbursts of irradiated accretion discs (King A.R.), 296, L45
LI Hot accretion discs with thermal Comptonization and advection in
\pparent superluminal expansion in Cygnus X-3 (Newell S.J., Garrett luminous black hole sources (Zdziarski A.A.), 296, L51
M.A., Spencer R.E.), 293, L17 Waves and instabilities in a differentially rotating disc containing a
The light curves of soft X-ray transients (King A.R., Ritter H.), 293, poloidal magnetic field (Ogilvie G.I.), 297, 291
L42 Simulations of superhumps and superoutbursts (Murray J.R.), 297, 323
The ultraviolet spectrum of the narrow-line Seyfert | galaxy RE The changing X-ray light curves of the intermediate polar FO Aquarii
J1034+396 (Puchnarewicz E.M., Mason K.O., Siemiginowska A.), (Beardmore A.P., Mukai K., Norton A.J., Osborne J.P., Hellier C.),
293, L52 297, 337
RX J1914.4 + 2456: the first double-degenerate polar? (Cropper M.., Soft X-ray transients in the Hertzsprung gap (Kolb U.), 297, 419
Harrop-Allin M.K., Mason K.O., Mittaz J.P.D., Potter S.B., Ramsay Iron Ka linewidths in magnetic cataclysmic variables (Hellier C.,
G.), 293, LS7 Mukai K., Osborne J.P.), 297, 526
Fast variability of the outflow in the Z CMa system (Chochol D., A general relativistic calculation of boundary layer and disc luminosity
Teodorani M., Strafella F., Errico L., Vittone A.A.), 293, L73 for accreting non-magnetic neutron stars in rapid rotation (Thampan
he circumnuclear material in the Galactic Centre: a clue to the A.V., Datta B.), 297, 570
accretion process (Sanders R.H.), 294, 35 Super-Eddington accretion discs around Kerr black holes
RX J0744—S2: a probable new intermediate polar (Ramsay G., (Beloborodov A.M.), 297, 739
Buckley D.A.H., Cropper M.), 294, 187 Photon bubbles in accretion discs (Gammie C.F.), 297, 929
Magnetic and vertical shear instabilities in accretion discs (Urpin V.., On the absence of jet features in the optical spectra of cataclysmic
Brandenburg A.), 294, 399 variables (Knigge C., Livio M.), 297, 1079
The radio—optical correlation in steep-spectrum quasars (Serjeant S.., The runaway instability of self-gravitating tori with non-constant
Rawlings S., Maddox S.J., Baker J.C., Clements D., Lacy M., Lilje specific angular momentum around black holes (Masuda N., Nishida
P.B.), 294, 494 S., Eriguchi Y.), 297, 1139
Effects of the Blandford—Znajek process on the evolution of the central ‘Stokes imaging’ of the accretion region in magnetic cataclysmic
black holes of accretion discs (Wang D.X., Lu Y., Yang L.T.), 294, variables — I. Conception and realization (Potter S.B., Hakala P.J.,
667 Cropper M.), 297, 1261
© 1998 RAS
Subject index
ymparison of white dwarf mass estimators using the intermediate Magnetospheric accretion and pre-main-sequence stellar masses
polar XY Ari (Ramsay G., Cropper M., Hellier C., Wu K.), 297, (Bonnell 1.A., Smith K.W., Meyer M.R., Tout C.A., Folha D.F.M
| hy Emerson J.P.), 299, 1013 .
Simulations of spiral structure in the accretion disc of IP Pegasi during Radiatively driven mass accretion on to galactic nuclei by
outburst (Armitage P.J.. Murray J.R.), 297, L81 circumnuclear starbursts (Umemura M., Fukue J., Mineshige S.)
Stellar dynamics in a galactic centre surrounded by a massive accretion 299, 1123
ian description (Vokrouhlicky D., Karas V.), 298, Eccentric instability of a two-dimensional fluid disc with a central
massive object (Taga M., lye M.), 299, 1132
structure around a magnetic neutron star: analytic and Magnetic reconnection: flares and coronal heating in active galactic
solutions (Brandenburg A., Campbell C.G.), 298, nuclei (Di Matteo T.), 299, L15
On the precession of accretion discs in X-ray binaries (Larwood J.)
u of Ha flares in AE Aquarii (Welsh W.F., Horne K 299, L32
298, 285 Echoes from an irradiated disc in GRO J1655—40 (Hynes R.L., O’ Brien
ervation of Cygnus X-1 — L. Spectral analysis (Dove J.B K., Horne K., Chen W., Haswell C.A.), 299, L37
ns J.. Nowak M.A., Vaughan B.A., Begelman M.C.), 298, 729 Variability associated with @ accretion disc theory for standard
ibsorption and reflection of a multitemperature advection-dominated discs (Blackman E.G.), 299, L48
tron—bremsstrahlung X-ray cooling shock in BY Cam (Done Three-dimensional numerical simulation of gaseous flow structure in
Maed7ziarz P.) 298, }3 semidetached binaries (Bisikalo D.V., Boyarchuk A.A., Chechetkin
aX isymmetric relativistic Bondi—Hoyle accretion on toa V.M., Kuznetsov O.A., Molteni D.), 300, 39
Schwarzschild black hole (Font J.A., Ibafiez J.M.), 298, 835 The 1996 outburst of GRO J1655—40: the challenge of interpreting the
Instability of spherical accretior 1. Shock-free Bondi accretion multiwavelength spectra (Hynes R.I., Haswell C.A., Shrader C.R
Kovalenko I.G., Eremin M.A.), 298, 861 hen W., Horne K., Harlaftis E.T., O’ Brien K., Hellier C., Fender
imit-cycle behaviour of thermally unstable accretion flowson to R.P.). 300, 64
black holes (Szuszkiewicz E., Miller J.( 298, 888 Magnetic field bending in accretion discs with dynamos (Campbell
Yu ion disc outbursts: a new version of an old model (Hameury C.G., Papaloizou J.C.B., Agapitou V.), 300, 315
J.-M., Menou K., DubusG ., Lasota J.-P., Huré J.-M.), 298, 1048 Tilted accretion discs in cataclysmic variables: tidal instabilities and
Slim accretion discs: a model for ADAF-—SLE transitions superhumps (Murray J.R., Armitage P_J.), 300, 561
1.V., Abramowicz M.A., Novikov I1.D.), 298, 1069 An RXTE observation of the Seyfert | galaxy MCG—6-30-15: X-ray
d spectra of the accretion disc and gas stream of reflection and the iron abundance (Lee J.C., Fabian A.C., Reynolds
iiable UX Ursae Majoris (Baptista R., Horne K C.S., lwasawa K., Brandt W.N.), 300, 583
Hubeny I., Long K.S., Rutten R.G.M.), 298, 1079 On spin-up/spin-down torque reversa mdi : reting nulsars (
cataclysmic variable period gap: still there (Kolb U., King A.R.., Wickramasinghe D.T.), 300, 1015
Ritter H.), 298, L29 An ‘outside-in’ outburst of Aql X-1 (Shahbaz T., Bandyopadhyay
Magnetic torques between ! m discs and stars (Torkelsson U.) R.M., Charles P.A., Wagner R.M., Muhli P., Hakala P., Casares J
298, L55 Greenhill J.), 300, 1035
Disc structure around s ¥ Magnetic accretors: a full disc solution Numerical simulations of protostellar encounters — I. Star—disc
vith turbulent diffusivity umpbell C.G., Heptinstall P.M.), 299, encounters (Boffin H.M.J., Watkins S.J., Bhattal A.S., Francis N
Whitworth A.P.), 300, 1189
olution of neutron stars uigh-mass ray binaries (Urpin V Numerical simulations of protostellar encounters — Il. Coplanar
Konenkov D., Geppert U.), 299, disc—dise encounters (Watkins S.J., Bhattal A.S., Boffin H.M.J
The new intermediate polar RX J1238—38: a system below the period Francis N., Whitworth A.P.), 300, 1205
zap? (Buckley D.A.H.., ¢ per M., RamsayG ., Wickramasinghe Numerical simulations of protostellar encounters — III. Non-coplanar
D.T.), 299, 83 disc—dise encounters (Watkins S.J., Bhattal A.S., Boffin H.M.J
ltrasoft X-ray components high-temperature extreme Francis N., Whitworth A.P.), 300, 1214
Puchnarewicz E.M.), 299, [ron line profiles including emission from within the innermost stable
Phase-resolved Hubble Space Telescope ultraviolet spectroscopy of orbit of a black hole accretion disc (Young A.J., Ross R.R., Fabian
V 795 Her (Rosen S.R., Prinja R.K., Drew J.E., Mason K.O., Howell A.C.), 300, L111
S.B.), 299, 305 On the spia paradigm and the radio dichotomy of quasars (Moderski
X-ray spectroscoy the broad-line radio galaxy 3C 111 (Reynold R., Sikora M., Lasota J.-P.), 301, 142
C.S., lwasawa K., Crawford C.S., Fabian A.C.), 299, 410 \ spectral decomposition of the variable optical, ultraviolet and X-ray
Comptonization and QPO origins in accreting neutron star systems continuum of NGC 5548 (Magdziarz P., Blaes O.M., Zdziarski
(Lee H.( Miller G.S.), 299, 479 4.A., Johnson W.N., Smith D.A.), 301, 179
Evidence for a rotational velocity field about the white dwarf of V347 The orbital period of HDE 226868/Cyg X-1 (LaSala J., Charles P.A
Puppis (Sull M.D., Buckley D.A.H., Garlick M.A.), 299, 545 Smith R.A.D., Batuciriska-Church M., Church M.J.), 301, 285
Spectroscopic evidence for two-pole accretion in the intermediate Soft X-ray transient light curves as standard candles: exponential
polar RX JOS558 + 5353 (Sull M.D., Duck S.R., Marsh T.R.), 299, versus linear decays (Shahbaz T., Charles P.A., King A.R.), 301,
59 382
rhe stream impact region in the disc of WZ Sge (Spruit H.C., Rutten Broad-band * -ray/y-ray spectra and binary parameters of GX 339-4
R.G.M.), 299, 768 and their astrophysical implications (Zdziarski A.A., Poutanen J.,
Smoothed particle hydrodynamic simulations of viscous accretion Mikotajewska J., Gierliriski M., Ebisawa K., Johnson W.N.), 301,
discs around black holes (LanzafameG ., Molteni D., Chakrabarti 435
S.K.), 299, 799 Disc structure around strongly magnetic accretors: a full disc solution
X-ray confirmationo f the new intermediate polar RX J1238—38 with buoyancy diffusivity (Campbell C.G., Heptinstall P.M.), 301,
(Hellier C., Beardmore A.P., Buckley D.A.H.), 299, 851 558
Oscillatory instability of radiative shocks with mulitiple cooling Stream overflow and dwarf nova eruptions (Schreiber M.R., Hessman
processes (Saxton C.J.. Wu K., Pongracic H., Shaviv G.), 299, 862 F.V.), 301, 626
4 double-frequency dwarf nova oscillation in OY Car (Marsh T.R., The chemical evolution of the secondary stars in close binaries, arising
Horne K.), 299, 921 from common-envelope evolution and nova outbursts (Marks P.B.,
\ ROSAT observation of the dipping, flaring and eclipsing polar MN Sarna M.J.), 301, 699
Hya (RX J0929. |—2404) (Buckley D.A.H., Barrett P.E., Haber! F.. Emission-line profiles from self-gravitating toroids around black holes
Sekiguchi K.), 299, 998 (Usui F., Nishida S., Eriguchi Y.), 301, 721
© 1998 RAS
Subject index
An analytic model for disc disruption by strong stellar magnetic fields Super-Eddington accretion discs around Kerr black holes
(( ampbell ¢ G.), 301, 754 (Beloborodov A.M.), 297, 739
Supermassive black holes in early-type galaxies: relationship with
Atomic data radio emission and constraints on the black hole mass function
Emission lines of [Ne tv] in the optical and ultraviolet spectrao f (Franceschini A., Vercellone S., Fabian A.C.), 297, 817
gaseous nebulae (Keenan F.P., Aller L.H., Bell K.L., Espey B.R The runaway instability of self-gravitating tori with non-constant
Feibelman W.A., Hyung S., McKenna F.C., Ramsbottom C.A.) specific angular momentum around black holes (Masuda N., Nishid:
295, 683 S., Eriguchi Y.), 297, 1139
The broadening of d—f and f—d transitions by collisions with neutral Non-axisymmetric relativistic Bondi—Hoyle accretion on toa
hydrogen atoms (Barklem P.S., O° Mara B.J.. Ross J.E.), 296, 1057 Schwarzschild black hole (Font J.A., [baéfiez J.M.). 298, 835
Solar EUV line identifications from delayed beam-foil spectra (Trabert Orbital motion of a massive object in a dense stellar system (Taga M
E.) 297. 399 lye M.), 299, 111
UV transitions of astrophysical interest in Ge, As 1 and Se 1 (Biémont Smoothed particle hydrodynamic simulations of viscous accretion
E., Morton D.C., Quinet P.), 297, 713 discs around black holes (Lanzafame G., Molteni D., Chakrabarti
The WC 10 central stars CPD—56° 8032 and He 2-113 — III. Wind S.K.), 299, 799
electron temperatures and abundances (De Marco O., Storey P.J., Radiatively driven mass accretion on to galactic nuclei by
Barlow M.J.), 297, 999 circumnuclear starbursts (Umemura M., Fukue J., Mineshige S.)
Recombination of helium-like ions — I. Photoionization cross-sections 299, 1123
and total recombination and cooling coefficients for atomic helium Resonant tidal disruption in galactic nuclei (Rauch K.P., Ingalls B.),
(Hummer D.G.., Storey P.J.), 297, 1073 299, 1231
Precise laboratory wavelengths of the Mgi and Mg ti resonance High-redshift galaxies, their active nuclei and central black holes
transitions at 2853, 2803 and 2796 A (Pickering J.C., Thorne A.P (Haehnelt M.G., Natarajan P., Rees M J.), 300, 817
Webb J.K.), 300, 131 Iron line profiles including emission from within the innermost stable
Accurate free—free Gaunt factors for astrophysical plasmas (Sutherland orbit of a black hole accretion disc (Young A.J., Ross R.R., Fabian
R.S.), 300, 321 A.C.), 300, L11
The 3s -S—4p -P® transition probability in Mg u (Fleming J., Hibbert A On the spin paradigm and the radio dichotomy of quasars (Moderski
Bell K.I Vaeck N.), 300, 767 R., Sikora M., Lasota J.-P.), 301, 142
The broadening of strong lines of Ca*, Mg* and Ba* by collisions Emission-line profiles from self-gravitating toroids around black holes
with neutral hydrogen atoms (Barklem P.S., O° Mara B.J.), 300, (Usui F., Nishida S., Eriguchi Y.), 301, 721
863
Photoionization from excited states of Ne1 (Seaton M.J.), 300, L1 Chaos
Anomalous mixing of the w -P°, and x °P®, levels in Fe | (Donnelly Lattice dynamical system modelling of molecular clouds (Rousseau
M.P.. Hibbert A.), 301, 809 G., Chaté H., Le Bourlot J.), 294, 373
Intermittent behaviour in axisymmetric mean-field dynamo models in
Atomic processes spherical shells (Tworkowski A., Tavakol R., Brandenburg A
Effective collision strengths for fine-structure forbidden transitions Brooke J.M., Moss D., Tuominen I.), 296, 287
among the 2s-2p° levels of Ne tv (Ramsbottom C.A., Bell K.1 Modulation and symmetry changes in stellar dynamos (Knobloch f
Keenan F.P.), 293, 233 Tobias S.M.. Weiss N.O.), 297, 1123
Electron impact excitation of the ground-state ’P fine-structure levels Three-body dynamics: intermittent chaos with strange attractor
in atomic oxygen (Bell K.L., Berrington K.A., Thomas M.R.J.), 293, (Heinaimaki P., Lehto H.J., Valtonen M.J., Chernin A.D.), 298, 790
L83 \ two-layer aw-dynamo model with dynamic feedback on the w-effect
H.,, formation on interstellar grains tn different physical regimes (Roald C.B.), 300, 397
(Biham O., Furnam I., Katz N., Pirronello V., Vidali G.), 296, 869 Phase mixing in time-independent Hamiltonian systems (Kandrup
UV transitions of astrophysical interest in Ge 1, Asti and Se 1 (Biémont H.E.), 301, 960
E., Morton D.C., Quinet P.), 297, 713
Recombinationo f helium-like ions — I. Photoionization cross-sections Conduction
and total recombination and cooling coefficients for atomic helium Self-inhibiting heat flux (Pistinner S.L., Eichler D.), 301, 49
(Hummer D.G.., Storey P.J.), 297, 1073
Accurate free—free Gaunt factors for astrophysical plasmas (Sutherland Convection
R.S.), 300, 321 4 note on the conditions for SSD—ADAF transitions (Abramowicz
M.A., lgumenshchev I. V., Lasota J.-P), 293, 443
Black hole physics \ numerical simulation of supersonic thermal convection (Dyt C.P
The radio—optical correlation in steep-spectrum quasars (Serjeant S Prentice A.J.R.), 296, 56
Rawlings S.. Maddox S.J., Baker J.C., Clements D.. Lacy M., Lily Evolution of DA white dwarfs in the context of a new theory of
P.B.), 294, 494 convection (Althaus L.G., Benvenuto O.G.), 296, 206
Effects of the Blandford—Znajek process on the evolution of the central On the validity of quasi-linear kinematic mean-field electrodynamics
black holes of accretion discs (Wang D.X., Lu Y., Yang L.T.), 294, in astrophysical flows (Petrovay K., Zsarg6 J.), 296, 245
667 Evolutionary sequences for Nova V1974 Cygni using new nuclear
On the magnetohydrodynamic description of a two-component plasma reaction rates and opacities (Starrfield S., Truran J.W., Wieschet
in the Kerr metric (Khanna R.), 294, 673 M.C., Sparks W.M.), 296, 502
Are Q-stars a serious threat for stellar-mass black hole candidates? The dependence of the diffusion coefficient on the mixing length in
(Miller J.C., Shahbaz T., Nolan L.A.), 294, L25 Kato’s overstable zone (Umezu M.), 298, 193
Global solutions of adiabatic accretion flows with isothermal shocks in Stellar evolution models for Z = 0.0001 to 0.03 (Pols O.R., Schrédet
Kerr black hole geometry (Lu J.-F., Yuan F.), 295, 66 K.-P., Hurley J.R., Tout C.A., Eggleton P.P.), 298, 525
Generation of magnetic fields by a gravitomagnetic plasma battery Effectso f errors in the solar radius on helioseismic inferences (Basu
(Khanna R.), 295, L6 S.), 298, 719
3+ 1 formulation of non-ideal hydrodynamics (Peitz J., App! S.), 296, Solar p-mode excitation: further insight from recent low-/ BiSON
231 helioseismological data (Chaplin W.J., Elsworth Y., Isaak G.R..,
Hot accretion discs with thermal Comptonization and advection in Lines R., McLeod C.P., Miller B.A., New R.), 298, L7
luminous black hole sources (Zdziarski A.A.), 296, L51 Modelling photospheric magnetoconvection (Blanchflower S.M.,
Soft X-ray transients in the Hertzsprung gap (Kolb U.), 297, 419 Rucklidge A.M., Weiss N.O.), 301, 593
1998 RAS
Subje f index
1e-dimensional magnetized relativistic pai
s (Marks P.B M.), 293, 44
M 1. yf artificia ity on a hydrodynamic mode
M.. Ishid Tanaka 294, 224
Cosmic strings Metal enrichment « wctic medium (Gnedin N.Y.), 294, 407
Global solutions o atic accretion flows with isothershmocaksl i n
Kerr black hok ymetry (Lu J.-F.. Yuan F.), 295, 66
4 cosmological h “dynamic code based on the piecewise parabolic
Dense matter method (Gheller Pantano O., Moscardini L.), 295,519
Radiation-driven winds from luminous accretion discs (Proga D
Stone J.M., Dr 295, 595
lose binary systems: a 3D SPH
me G., Belveder ), 295, 618
ooling resulting trom luminous
Diffusion tuko N Habe \ sibasi N 295,
cular clump
295, 738
Im )possiDi«
io M., I
Hydrodynamiofc sth e
.Y., Hui L.), 296, 44
Elementary particles
Equation of state tion disc of the
‘> K.), 296, 463
‘A
Gravitation ised by 1
J.M., O’Brein T.J., Bode M.I
ul
lel for massive
1.M.), 296, L6
ri oO c DM hydrodynamical
P B., Dominguez-T eiro R.), 297, 177
Stabilit } lifferentially rotati
G.1.}, 297, 291
perhumps and superoutbursts (Murray J.R.) 297, 323
yn to th e hypersonic, radiative blunt body problem
297. ~ 4
convenient set of comoving cosmological variables and thei
ipplication (Martel H., Shapiro P.R.), 297, 46
Super-Eddington accretion discs around Kerr black hol
(Beloborodov A.M.), 297, 739
Galaxy formation and evolution — |. The Padua
(CarraroG ., Lia ¢ iosi C.), 297, 1021
Pattern speed of the stellar bar in NGC 7479 (Laine S., Shlosman |
Heller C.H.), 297, 1052
The large-scale structure of FR-II radio sources (Komis
Falle S.A.E.G.), 297, 108
The low-redshift evolution of the an-a { eun I eonard
Montero M.), 301, 4... Efstathiou G.), 297, L49
Simulations of spiral structure in the accretion disc of IP Pegasi during
outburst (Armitage P.J.. Murray J.R.), 297, L81
Cometary and bipolar ultracompact H 1 regions (Redman M.P
tructul nerated Dy nuciear starDursts Williams R.J.R., Dyson J.E.), 298, 33
Mufioz-Tufién ¢ 293, 299 Numerical simulationso f rotating cooling flows in galaxy cluster
4 note on the conditions for SSD—ADAF transitions (Abramowicz environments (Garasi C., Loken C., Burns J.0., Roettiger K.), 298,
M.A.., Igumenshchev 1.V ., Lasota J.-P), 293, 443 697
1998 RAS