Vocabulary for Astronomy & Astrophysics Journal keywords (Version wd-1.0)
Acceleration of particles
Accretion, accretion disks
Astrobiology
Astrochemistry
Astrometry
Astrometry and celestial mechanics
Astronomical data bases
Astronomical data bases: miscellaneous
Astronomical instrumentation, methods and techniques
Atlases
Atmospheric effects
Atomic data
Atomic processes
Balloons
Black hole physics
Catalogs
Celestial mechanics
Chaos
Comets: general
Conduction
Convection
Cosmology
CMB
Cosmic microwave background
Cosmological parameters
Dark matter
Diffuse radiation
Distance scale
Early universe
Large-scale structure of Universe
Cosmology: miscellaneous
Cosmology: observations
Cosmology: theory
Dense matter
Diffusion
Earth
Eclipses
Elementary particles
Ephemerides
Equation of state
Galaxies
Galaxies: abundances
Galaxies: active
BL Lacertae objects: general
Galaxies: bulges
Galaxies: clusters: general
Cooling flows
Galaxies: distances and redshifts
Galaxies: dwarf
Galaxies: elliptical and lenticular, cD
Galaxies: evolution
Galaxies: formation
Galaxies: fundamental parameters
Classification, colors, luminosities, masses, radii, temperatures, etc.
Galaxies: general
Galaxies: halos
Galaxies: high-redshift
Galaxies: interactions
IGM
Intergalactic medium
Galaxies: irregular
Galaxies: ISM
Galaxies: jets
Galaxies: kinematics and dynamics
Local Group
Galaxies: luminosity function, mass function
LMC
SMC
Magellanic Clouds
Galaxies: magnetic fields
Galaxies: nuclei
Galaxies: peculiar
Galaxies: photometry
Quasars: absorption lines
Quasars: emission lines
Quasars: general
Galaxies: Seyfert
Galaxies: spiral
Galaxies: star clusters
Galaxies: starburst
Galaxies: statistics
Galaxies: stellar content
Galaxies: structure
Galaxy: abundances
Galaxy: bulge
Galaxy: center
Galaxy: disk
Galaxy: evolution
Galaxy: formation
Galaxy: fundamental parameters
Galaxy: general
Globular clusters: general
Galaxy: halo
Galaxy: kinematics and dynamics
Galaxy: nucleus
Open clusters and associations:general
Solar neighbourhood
Galaxy: stellar content
Galaxy: structure
GRB
Gamma rays: bursts
Gamma rays: observations
Gamma rays: theory
Gravitation
Gravitational lensing
Gravitational waves
Hydrodynamics
Infrared: galaxies
Infrared: general
Infrared: ISM
Infrared: solar system
Infrared: stars
Instabilities
Instrumentation: adaptive optics
Instrumentation: detectors
Instrumentation: high angular resolution
Instrumentation: interferometers
Instrumentation: miscellaneous
Instrumentation: photometers
Instrumentation: polarimeters
Instrumentation: spectrographs
Interplanetary medium
ISM, nebulae
Interstellar medium, nebulae
ISM: abundances
ISM: atoms
ISM: bubbles
ISM: clouds
Cosmic rays
Dust, extinction
Evolution
ISM: general
Herbig-Haro objects
HII regions
ISM: jets and outflows
ISM: kinematics and dynamics
ISM: lines and bands
ISM: magnetic fields
ISM: molecules
Planetary nebulae: general
Reflection nebulae
ISM: structure
SNR
ISM: supernova remnants
Kuiper Belt
Light pollution
Line: formation
Line: identification
Line: profiles
Magnetic fields
Magnetohydrodynamics
MHD
Masers
Meteors, meteoroids
Methods: analytical
Methods: data analysis
Methods: laboratory
Methods: miscellaneous
Methods: N-body simulations
Methods: numerical
Methods: observational
Methods: statistical
Minor planets, asteroids
Molecular data
Molecular processes
Moon
Neutrinos
Nuclear reactions, nucleosynthesis, abundances
Occultations
Oort Cloud
Physical data and processes
Planets and satellites: formation
Planets and satellites: general
Planets: rings
Plasmas
Polarization
Radiation mechanisms: general
Radiation mechanisms: non-thermal
Radiation mechanisms: thermal
Radiative transfer
Radio continuum: galaxies
Radio continuum: general
Radio continuum: ISM
Radio continuum: solar system
Radio continuum: stars
Radio lines: galaxies
Radio lines: general
Radio lines: ISM
Radio lines: solar system
Radio lines: stars
Reference systems
Relativity
Scattering
Shock waves
Site testing
Solar system
Solar system: formation
Solar system: general
Sources as a function of wavelength
Space vehicles
Space vehicles: instruments
Stars
Stars: abundances
Stars: activity
AGB
post-AGB
Stars: AGB and post-AGB
Stars: atmospheres
Binaries: close
Binaries: eclipsing
Binaries: general
Binaries: spectroscopic
Binaries: symbiotic
Binaries: visual
Blue stragglers
Stars: carbon
Stars: chemically peculiar
Stars: chromospheres
Circumstellar matter
Stars: coronae
Stars: distances
star.variable.UGem-class
Stars: dwarf novae
Stars: early-type
Stars: emission-line, Be
Stars: evolution
Stars: flare
Stars: formation
Stars: fundamental parameters
Stars: general
Color-Magnitude diagrams
H-R and C-M diagrams
H-R and CM diagrams
HR and C-M diagrams
HR and CM diagrams
Hertzsprung-Russel and Color-Magnitude diagrams
Hertzsprung-Russel diagrams
Hertzsprung-Russell and C-M diagrams
Stars: horizontal-branch
Stars: imaging
Stars: interiors
Stars: kinematics
Stars: late-type
Stars: low-mass, brown dwarfs
Stars: luminosity function, mass function
Stars: magnetic fields
Stars: mass-loss
Stars: neutron
Novae, cataclysmic variables
Stars: oscillations
Stars: peculiar
Planetary systems
Planetary systems: formation
proplyd
Planetary systems: protoplanetary disks
Stars: Population II
PMS
Stars: pre-main sequence
Pulsars: general
Stars: rotation
Starspots
Stars: statistics
Subdwarfs
Supergiants
Supernovae: general
Cepheids
Delta Sct
Stars: variables: general
Stars: variables: RR Lyr
White dwarfs
Stars: winds, outflows
Stars: Wolf-Rayet
Stellar dynamics
Submillimeter
Sun: abundances
Sun: activity
Sun: atmosphere
Sun: chromosphere
Sun: corona
CMEs
Sun: coronal mass ejections
Sun: evolution
Sun: faculae, plages
Sun: filaments
Sun: flares
Sun: fundamental parameters
Sun: general
Sun: granulation
Sun: helioseismology
Sun: infrared
Sun: interior
Sun: magnetic fields
Sun: oscillations
Sun: particle emission
Sun: photosphere
Sun: prominences
Sun: radio radiation
Sun: rotation
Solar wind
Solar-terrestrial relations
Sunspots
Sun: transition region
Sun: UV radiation
Sun: X-rays, gamma rays
Surveys
Techniques: high angular resolution
Techniques: image processing
Techniques: interferometric
Techniques: miscellaneous
Techniques: photometric
Techniques: polarimetric
Techniques: radar astronomy
Techniques: radial velocities
Techniques: spectroscopic
Telescopes
The Galaxy
The Sun
Time
Turbulence
Ultraviolet: galaxies
Ultraviolet: general
Ultraviolet: ISM
Ultraviolet: solar system
Ultraviolet: stars
Waves
X-rays: binaries
X-rays: bursts
X-rays: diffuse background
X-rays: galaxies
X-rays: galaxies: clusters
X-rays: general
X-rays: ISM
X-rays: stars
Line
Radiation mechanisms
Instrumentation
Methods
Techniques
Comets
Comets: individual
Planets
Planets and satellites
Planets and satellites: individual
Stars: Binaries
Stars: individual
Stars: Planetary systems
Stars: Pulsars
(Stars:) pulsars: individual
Stars: Supernovae
(Stars:) supernovae: individual
Stars: Variables
Interstellar medium
ISM: individual objects (except planetary nebulae)
ISM: Planetary nebulae
(ISM:) planetary nebulae: individual
Galaxy
Galaxy: Globular clusters
(Galaxy:) globular clusters: individual
Galaxy: Open clusters and associations
(Galaxy:) open clusters and associations:individual
Galaxies: BL Lacertae objects
(Galaxies:) BL Lacertae objects: individual
Galaxies: Clusters
Galaxies: clusters: indiviuals
Galaxies: individual
Galaxies: Quasars
(Galaxies:) quasars: individual
Gamma rays
Infrared
Radio continuum
Radio lines
Ultraviolet
X-rays
X-rays: individuals