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- \input aa.cmm
- \titlea{The thirteen sections}
- \halign{\hfil#\quad\hfill\cr
- 1.& Letters \cr
- 2.& Cosmology \cr
- 3.& Extragalactic astronomy \cr
- 4.& Galactic structures and dynamics \cr
- 5.& Stellar clusters and dynamics \cr
- 6.& Formations, structures and evolution \cr
- & of stars \cr
- 7.& Stellar atmospheres \cr
- 8.& Diffuse matter in space (including \cr
- & H\,{\sc II} regions and planetary nebulae) \cr
- 9.& the Sun \cr
- 10.& the solar system \cr
- 11.& Celestial mechanics and astrometry \cr
- 12.& Physical and chemical processes \cr
- 13.& Instruments, data processing, and \cr
- & computational methods \cr}
- %
- \titlea{Thesaurus of key words used in the annual subject indexes
- {\rm revised November 1989}}
- {\bf N.B.} The key words listed under the code numbers 07.11.1, 09.11.1,
- 09.16.1, 09.22.1, 16.03.1, 16.07.1, 16.14.1, 17.02.1, 19.42.1 and
- 19.93.1 are intended for use with specific astronomical objects; each
- contains the word ``individual". The corresponding code numbers should
- never be used alone, but always in combination with the most common
- names for the astronomical objects in question. For example, if a paper
- discusses three individual galaxies, these should be coded on the title
- page of the manuscript in the following manner: \par
- 07.11.1 Arp 220; 07.11.1 M 51; 07.11.1 NGC 4472\par\noindent
- Note that {\it each object} (in the example the three galaxies) counts
- as {\it one} Thesaurus code. No more than {\it six} codes all together
- should be listed as this is the limit fixed by the computer program.
- \bigskip
- \setbox0=\hbox{01.01.1\quad}\lindent=\wd0\relax
- \def\litem{\goodbreak\noindent\hangindent=\lindent\ltextindent}%
- \litem{} Absolute magnitudes; {\it see Stars: luminosities of}
- \litem{} Abundances; {\it see under the different objects}
- \litem{01.01.1} Acceleration mechanisms
- \litem{01.01.2} Accretion, accretion disks
- \litem{01.02.1} Analytical methods
- \litem{} Associations; {\it see Clusters: open, and associations}
- \litem{01.03.1} Asteroids
- \litem{01.04.1} Astrometry
- \litem{01.05.1} Astronomical constants
- \litem{01.06.1} Atlases
- \litem{01.07.1} Atomic and molecular data
- \litem{01.08.1} Atomic and molecular processes; {\it see also Chemical
- reactions}
- \litem{01.08.2} Background radiations
- \litem{} Binary stars; {\it see Stars: binaries}
- \medbreak
- \litem{02.01.1} BL Lacertae objects
- \litem{02.02.1} Black holes
- \medbreak
- \litem{03.01.1} Catalogues and dictionaries
- \litem{03.02.1} Celestial mechanics
- \litem{03.03.1} Chemical reactions
- \litem{03.04.1} Clusters: of galaxies
- \litem{03.05.1} Clusters: globular
- \litem{03.06.1} Clusters: open, and associations
- \litem{} Collisions, atomic and molecular; {\it see Atomic and
- molecular data}
- \litem{03.07.1} Comets
- \litem{03.08.1} Convection
- \litem{03.10.1} Cosmic rays; {\it see also Sun (the): cosmic rays}
- \litem{03.11.1} Cosmogony
- \litem{03.12.1} Cosmology
- \litem{03.12.2} Dark matter
- \medbreak
- \litem{04.01.1} Data analysis; {\it see also Image processing}
- \litem{04.02.1} Dense matter
- \litem{04.03.1} Distances, distance scale
- \litem{} Double stars; {\it see Stars: binaries}
- \litem{} Dust; {\it see Interstellar medium: dust; Interplanetary
- medium}
- \medbreak
- \litem{05.01.1} Earth: atmosphere
- \litem{05.02.1} Earth: general
- \litem{05.02.2} Earth: rotation
- \litem{05.03.1} Eclipses
- \litem{05.04.1} Editorials
- \litem{05.06.1} Elementary particles
- \litem{05.07.1} Ephemerides
- \litem{05.08.1} Errata
- \medbreak
- \litem{06.01.1} Fundamental stars and other objects
- \medbreak
- \litem{07.01.1} Galaxies: active; {\it see also Galaxies, Seyfert;
- Galaxies: nuclei of; Quasars}
- \litem{07.02.1} Galaxies: barred
- \litem{} Galaxies: clusters of, {\it see Clusters: of galaxies}
- \litem{07.03.1} Galaxies: compact
- \litem{07.05.1} Galaxies: dwarf elliptical
- \litem{07.06.1} Galaxies: elliptical
- \litem{07.07.1} Galaxies: evolution of
- \litem{07.08.1} Galaxies: formation of
- \litem{07.09.1} Galaxies: general
- \litem{07.10.1} Galaxies: haloes of
- \litem{07.11.1} Galaxies: individual; {\it see also Galaxies: Magellanic
- Clouds}
- \litem{07.12.1} Galaxies: irregular
- \litem{07.13.1} Galaxies: jets of
- \litem{07.14.1} Galaxies: kinematics and dynamics of
- \litem{07.15.1} Galaxies: lenticular
- \litem{07.16.1} Galaxies: Magellanic Clouds
- \litem{07.17.1} Galaxies: radio
- \litem{07.18.1} Galaxies: nuclei of
- \litem{07.19.1} Galaxies: redshifts of
- \litem{07.20.1} Galaxies: Seyfert
- \litem{07.21.1} Galaxies: spiral
- \litem{07.22.1} Galaxies: stellar content of
- \litem{07.23.1} Galaxies: structure of
- \litem{07.24.1} Galaxy (the): bulge of
- \litem{07.25.1} Galaxy (the): center of
- \litem{07.27.1} Galaxy (the): disk of
- \litem{07.28.1} Galaxy (the): evolution of
- \litem{07.29.1} Galaxy (the): general
- \litem{07.30.1} Galaxy (the): halo of
- \litem{07.31.1} Galaxy (the): kinematics and dynamics of
- \litem{07.32.1} Galaxy (the): solar neighbourhood
- \litem{07.33.1} Galaxy (the): stellar content of
- \litem{07.34.1} Galaxy (the): structure of
- \litem{07.35.1} Gamma rays: bursts
- \litem{07.36.1} Gamma rays: general
- \litem{} Gas dynamcis; {\it see Hydrodynamics and hydromagnetics}
- \litem{} Grains; {\it see Interstellar medium: dust; Interplanetary
- medium}
- \litem{07.37.1} Gravitation
- \litem{07.37.2} Herbig-Haro objects
- \medbreak
- \litem{08.01.1} Hydrodynamics
- \litem{08.02.1} Hydromagnetics
- H{\petit II} regions; {\it see Interstellar medium:
- H{\petit II} regions}
- \medbreak
- \litem{09.01.1} Image processing
- \litem{09.02.1} Infrared radiation
- \litem{09.03.1} Instruments; {\it see also: Interferometry; Radio telescopes;
- Space vehicles}
- \litem{09.04.1} Interferometry
- \litem{09.05.1} Intergalactic medium
- \litem{09.06.1} Interplanetary medium
- \litem{09.07.1} Interstellar medium: abundances
- \litem{09.08.1} Interstellar medium: bubbles
- \litem{09.09.1} Interstellar medium: clouds: general
- \litem{09.10.1} Interstellar medium: clouds: high velocity
- \litem{09.11.1} Interstellar medium: clouds: individual
- \litem{09.12.1} Interstellar medium: dust
- \litem{09.13.1} Interstellar medium: extinction
- \litem{09.14.1} Interstellar medium: general
- \litem{09.15.1} Interstellar medium: H{\petit II} regions: general
- \litem{09.16.1} Interstellar medium: H{\petit II} regions: individual
- \litem{09.17.1} Interstellar medium: kinematics and dynamics of
- \litem{09.18.1} Interstellar medium: magnetic field
- \litem{09.19.1} Interstellar medium: molecules
- \litem{} Interstellar medium: planetary nebulae; {\it see Planetary
- nebulae}
- \litem{09.20.1} Interstellar medium: radiation field
- \litem{09.21.1} Interstellar medium: reflection nebulae: general
- \litem{09.22.1} Interstellar medium: reflection nebulae: individual
- \litem{} Interstellar medium: shells; {\it see Interstellar medium:
- bubbles}
- \litem{} Interstellar medium: supernova remnants;
- {\it see Supernovae and supernova remnants}
- \medbreak
- \litem{12.01.1} Lines: formation; {\it see also: Radiation transfer}
- \litem{12.02.1} Lines: identification
- \litem{12.03.1} Lines: profile
- \litem{12.04.1} Luminosity function, mass function
- \medbreak
- \litem{} Magellanic Clouds: {\it see Galaxies: Magellanic Clouds}
- \litem{13.01.1} Magnetic field
- \litem{} Magnetohydrodynamics; {\it see Hydromagnetics, plasmas}
- \litem{13.02.1} Masers
- \litem{} Mass function; {\it see Luminosity function, mass function}
- \litem{13.03.1} Meteors, meteorites
- \litem{} Microwave background; {\it see Cosmic background
- radiation}
- \litem{} Molecules; {\it see Atomic and molecular data; Interstellar
- medium: molecules; Radio lines: molecular}
- \litem{} Nebulae; {\it see Interstellar medium: H{\petit II} regions; Planetary
- nebulae; Interstellar medium: reflection nebulae; Supernovae and
- supernova remnants}
- \litem{} Neutrinos; {\it see Elementary particles}
- \medbreak
- \litem{14.01.1} Nuclear reactions
- \litem{14.02.1} Nucleosynthesis
- \litem{14.03.1} Numerical methods
- \medbreak
- \litem{15.01.1} Observational methods
- \litem{15.02.1} Occultations
- \litem{} Parallaxes; {\it see Distances, distance scale}
- \litem{} Particle acceleration; {\it see Acceleration mechanisms}
- \medbreak
- \litem{16.01.1} Photometry
- \litem{16.02.1} Planetary nebulae: general
- \litem{16.03.1} Planetary nebulae: individual
- \litem{16.04.1} Planets and satellites: abundances
- \litem{16.05.1} Planets and satellites: atmospheres of
- \litem{16.06.1} Planets and satellites: general
- \litem{16.07.1} Planets and satellites: individual
- \litem{16.08.1} Planets and satellites: magnetospheres of
- \litem{16.09.1} Planets and satellites: Moon
- \litem{16.09.2} Planets and satellites: rings
- \litem{16.10.1} Planets and satellites: satellites
- \litem{16.11.1} Plasmas
- \litem{16.12.1} Polarization
- \litem{} Positions; {\it see Astrometry; Fundamental stars and other
- objects}
- \litem{} Proper motions; {\it see Astrometry; Fundamental stars and
- other objects}
- \litem{} Protostars; {\it see Stars: pre-main-sequence; Interstellar
- medium: clouds; Interstellar medium: kinematics and
- dynamics of}
- \litem{16.13.1} Pulsars: general
- \litem{16.14.1} Pulsars: individual
- \medbreak
- \litem{17.01.1} Quasars: general
- \litem{17.02.1} Quasars: individual
- \litem{17.03.1} Quasars: jets of
- \litem{17.04.1} Quasars: redshifts of
- \medbreak
- \litem{18.01.1} Radar astronomy
- \litem{18.02.1} Radial velocities: {\it see also Galaxy (the): kinematics and
- dynamics of; Galaxies: redshifts of; Quasars: redshift of}
- \litem{18.03.1} Radiation mechanisms: general
- \litem{18.03.2} Radiation mechanisms: synchrotron radiation
- \litem{18.04.1} Radiation transfer; {\it see also Lines, formation}
- \litem{} Radio galaxies; {\it see Galaxies, radio}
- \litem{18.05.1} Radio lines: molecular
- \litem{18.06.1} Radio lines: recombination
- \litem{18.07.1} Radio lines: 21-cm
- \litem{18.08.1} Radio sources: general; {\it see also individual objects}
- \litem{18.08.2} Radio continuum
- \litem{18.09.1} Radio telescopes
- \litem{18.09.2} Reference systems
- \litem{18.10.1} Relativity
- \medbreak
- \litem{19.01.1} Satellites; {\it see Planets and satellites}
- \litem{19.02.1} Scintillation
- \litem{19.03.1} Seeing
- \litem{19.04.1} Shock waves
- \litem{19.05.1} Site testing
- \litem{} Solar neighbourhood: {\it see Galaxy (the): solar
- neighbourhood}
- \litem{19.06.1} Solar system: general
- solar wind; {\it see Interplanetary medium}
- \litem{19.07.1} Space vehicles and instruments
- \litem{19.08.1} Spectrophotometry
- \litem{19.09.1} Spectroscopy
- \litem{} Spiral structure: {\it see Galaxy (the): kinematics and
- dynamics of; Galaxy (the): structure of; Galaxies:
- kinematics and dynamics of; Galaxies: spiral; Galaxies:
- structure of}
- \litem{19.10.1} Stars: abundances
- \litem{19.11.1} Stars: activity of
- \litem{19.12.1} Stars: atmospheres of
- \litem{19.13.1} Stars: Be
- \litem{19.14.1} Stars: $\beta$ Cep
- \litem{19.15.1} Stars: binaries: close
- \litem{19.16.1} Stars: binaries: general
- \litem{19.17.1} Stars: binaries: spectroscopic
- \litem{19.18.1} Stars: binaries: symbiotic
- \litem{19.19.1} Stars: binaries: visual
- \litem{19.20.1} Stars: blue stragglers
- \litem{19.21.1} Stars: bolometric correction
- \litem{19.22.1} Stars: carbon
- \litem{} Stars: cataclysmic variables; {\it see Stars: novae}
- \litem{19.23.1} Stars: Cepheids
- \litem{19.24.1} Stars: chromospheres of
- \litem{19.25.1} Stars: circumstellar matter
- \litem{19.25.2} Stars: chemical peculiar
- \litem{19.26.1} Stars: classification
- \litem{19.27.1} Stars: collapsed
- \litem{19.28.1} Stars: colors of
- \litem{19.29.1} Stars: coronae of
- \litem{19.30.1} Stars: diameters of
- \litem{19.31.1} Stars: $\delta$ Sct
- \litem{19.31.2} Stars: dynamics
- \litem{19.31.3} Stars: dwarfs
- \litem{19.32.1} Stars: early-type
- \litem{19.33.1} Stars: emission-line
- \litem{19.34.1} Stars: evolution of
- \litem{19.35.1} Stars: faint blue
- \litem{19.36.1} Stars: flare
- \litem{19.37.1} Stars: formation of
- \litem{19.38.1} Stars: general
- \litem{19.39.1} Stars: giant
- \litem{19.40.1} Stars: helium
- \litem{19.41.1} Stars: Hertzsprung-Russell diagram
- \litem{19.42.1} Stars: individual
- \litem{} Stars: interior; {\it see Stars: structure of}
- \litem{19.43.1} Stars: late-type
- \litem{19.44.1} Stars: long-period variables
- \litem{19.45.1} Stars: luminosities of
- \litem{19.46.1} Stars: magnetic field
- \litem{19.47.1} Stars: mass of
- \litem{19.48.1} Stars: mass loss
- \litem{19.49.1} Stars: mass-luminosity relation
- \litem{} Stars: Mira; {\it see Stars: long-period variables}
- \litem{19.50.1} Stars: neutron
- \litem{19.51.1} Stars: novae and cataclysmic variables
- \litem{19.52.1} Stars: OH/IR
- \litem{19.53.1} Stars: oscillations of
- \litem{19.55.1} Stars: Population I
- \litem{19.56.1} Stars: Population II
- \litem{19.57.1} Stars: Population III
- \litem{19.58.1} Stars: pre-main-sequence
- \litem{19.59.1} Stars: radio radiation of
- \litem{19.60.1} Stars: rotation of
- \litem{19.61.1} Stars: RR Lyr
- \litem{19.62.1} Stars: runaway
- \litem{19.63.1} Stars: structure of
- \litem{19.64.1} Stars: subdwarf
- \litem{19.65.1} Stars: supergiant
- \litem{} Stars: supernovae; {\it see Supernovae and supernova}
- remnants
- \litem{19.66.1} Stars: temperatures of
- \litem{} Stars: T Tau; {\it see Stars: pre-main-sequence}
- \litem{19.67.1} Stars: variable
- \litem{19.68.1} Stars: white dwarf
- \litem{} Stars: winds; {\it see Stars: mass loss}
- \litem{19.69.1} Stars: Wolf-Rayet
- \litem{} Submillimetre radiation; {\it see Infrared radiation}
- \litem{19.70.1} Sun (the): abundances
- \litem{19.71.1} Sun (the): activity of
- \litem{19.72.1} Sun (the): atmosphere of
- \litem{19.73.1} Sun (the): bursts
- \litem{19.74.1} Sun (the): chromosphere of
- \litem{19.75.1} Sun (the): corona of
- \litem{19.76.1} Sun (the): cosmic rays
- \litem{19.77.1} Sun (the): faculae
- \litem{19.78.1} Sun (the): flares
- \litem{19.79.1} Sun (the): general
- \litem{19.80.1} Sun (the): granulation
- \litem{} Sun (the): {\it see Sun (the): structure of}
- \litem{19.81.1} Sun (the): magnetic fields
- \litem{19.82.1} Sun (the): oscillations of
- \litem{19.83.1} Sun (the): photosphere of
- \litem{19.84.1} Sun (the): prominences
- \litem{19.85.1} Sun (the): radio radiation of
- \litem{19.86.1} Sun (the): rotation of
- \litem{19.87.1} Sun (the): solar-terrestrial relations;
- {\it see also Interplanetary medium}
- \litem{19.88.1} Sun (the): solar wind; {\it see also Interplanetary medium}
- \litem{19.89.1} Sun (the): structure of
- \litem{19.90.1} Sun (the): sunspots
- \litem{19.91.1} Sun (the): X-rays
- \litem{19.92.1} Supernovae and supernova remnants: general
- \litem{19.93.1} Supernovae and supernova remnants: individual
- \litem{19.94.1} Surveys
- \litem{} Synchrotron radiation; {\it see Radiation mechanisms}
- \litem{19.95.1} Time
- \litem{} Transition probabilities: {\it see Atomic and molecular data}
- \medbreak
- \litem{20.01.1} Turbulence
- \litem{20.01.2} Universe (the): structure of
- \medbreak
- \litem{21.01.1} UV radiation; {\it see also under the different objects}
- \medbreak
- \litem{24.01.1} X-rays: binaries
- \litem{24.02.1} X-rays: bursts
- \litem{24.03.1} X-rays: general
- \litem{24.04.1} X-rays: spectroscopy
- \bye