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AAS Subject Key Words

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AAS Subject Key Words

as of 3/16/012


Authors should select subject key words for their manuscripts using the list given below. No more than six key words should
be given (and if key words are used for individual stars, galaxies, etc., each object normally counts as one key word). The overall categories (which are capitalized) should not be included. Also, do not include any part of a key word that is in parentheses (marked in italic below): thus, (stars:) binaries (including multiple): close should be given as binaries: close. The key words should be listed in alphabetical order after the abstract as in the following example:

Key Words: Cepheids --- galaxies: individual (M100, NGC 4321) --- stars: early type

Headings such as galaxies: individual (..., ...) should include the individual names in parentheses, as indicated above.

Note that in RevMexAA macros, the \addkeyword{text} command for subject key words must be placed after the \abstract{text} command and not before it.

Subject Key Words List

    Physical Data and Processes
    Astronomical Instrumentation, Methods, and Techniques
    Astronomical Databases
    Astrometry and Celestial Mechanics
    The Sun
    Planetary Systems
    Interstellar Medium (ISM), Nebulae
    The Galaxy
    Resolved and Unresolved Sources as a Function of Wavelength


editorials, notices
errata, addenda
extraterrestrial intelligence
history and philosophy of astronomy
obituaries, biographies
publications, bibliography
sociology of astronomy

Physical Data and Processes

acceleration of particles
accretion, accretion disks
astroparticle physics
atomic data
atomic processes
black hole physics
dense matter
elementary particles
equation of state
gravitational lensing: strong
gravitational lensing: weak
gravitational lensing: micro
gravitational waves
line: formation
line: identification
line: profiles
magnetic fields
magnetic reconnection
magnetohydrodynamics (MHD)
molecular data
molecular processes
nuclear reactions, nucleosynthesis, abundances
radiation mechanisms: general
radiation mechanisms: non-thermal
radiation mechanisms: thermal
radiative transfer
relativistic processes
shock waves

Astronomical Instrumentation, Methods, and Techniques

atmospheric effects
instrumentation: adaptive optics
instrumentation: detectors
instrumentation: high angular resolution
instrumentation: interferometers
instrumentation: miscellaneous
instrumentation: photometers
instrumentation: polarimeters
instrumentation: spectrographs
light pollution
methods: analytical
methods: data analysis
methods: laboratory
methods: miscellaneous
methods: numerical
methods: observational
methods: statistical
site testing
space vehicles
space vehicles: instruments
techniques: high angular resolution
techniques: image processing
techniques: imaging spectroscopy
techniques: interferometric
techniques: miscellaneous
techniques: photometric
techniques: polarimetric
techniques: radar astronomy
techniques: radial velocities
techniques: spectroscopic

Astronomical Databases

astronomical databases: miscellaneous
virtual observatory tools

Astrometry and Celestial Mechanics

celestial mechanics
proper motions
reference systems

The Sun

Sun: abundances
Sun: activity
Sun: atmosphere
Sun: chromosphere
Sun: corona
Sun: coronal mass ejections (CMEs)
Sun: dynamo
Sun: evolution
Sun: faculae, plages
Sun: filaments, prominences
Sun: flares
Sun: fundamental parameters
Sun: general
Sun: granulation
Sun: helioseismology
Sun: heliosphere
Sun: infrared
Sun: interior
Sun: magnetic topology
Sun: oscillations
Sun: particle emission
Sun: photosphere
Sun: radio radiation
Sun: rotation
(Sun:) solar–terrestrial relations
(Sun:) solar wind
(Sun:) sunspots
Sun: surface magnetism
Sun: transition region
Sun: UV radiation
Sun: X-rays, gamma rays

Planetary Systems

comets: general
comets: individual (..., ...)
interplanetary medium
Kuiper belt: general
Kuiper belt objects: individual (..., ...)
meteorites, meteors, meteoroids
minor planets, asteroids: general
minor planets, asteroids: individual (..., ...)
Oort Cloud
planets and satellites: atmospheres
planets and satellites: aurorae
planets and satellites: composition
planets and satellites: detection
planets and satellites: dynamical evolution and stability
planets and satellites: formation
planets and satellites: fundamental parameters
planets and satellites: general
planets and satellites: individual (..., ...)
planets and satellites: interiors
planets and satellites: magnetic fields
planets and satellites: physical evolution
planets and satellites: rings
planets and satellites: surfaces
planets and satellites: tectonics
protoplanetary disks
planet–disk interactions
planet–star interactions
zodiacal dust


stars: abundances
stars: activity
stars: AGB and post-AGB
stars: atmospheres
(stars:) binaries (including multiple): close
(stars:) binaries: eclipsing
(stars:) binaries: general
(stars:) binaries: spectroscopic
(stars:) binaries: symbiotic
(stars:) binaries: visual
(stars:) blue stragglers
(stars:) brown dwarfs
stars: carbon
stars: chemically peculiar
stars: chromospheres
(stars:) circumstellar matter
stars: coronae
stars: distances
stars: dwarf novae
stars: early-type
stars: emission-line, Be
stars: evolution
stars: flare
stars: formation
stars: fundamental parameters
stars: general
(stars:) gamma-ray burst: general
(stars:) gamma-ray burst: individual (..., ...)
(stars:) Hertzsprung–Russell and C–M diagrams
stars: horizontal-branch
stars: imaging
stars: individual (..., ...)
stars: interiors
stars: kinematics and dynamics
stars: late-type
stars: low-mass
stars: luminosity function, mass function
stars: magnetars
stars: magnetic field
stars: massive
stars: mass-loss
stars: neutron
(stars:) novae, cataclysmic variables
stars: oscillations (including pulsations)
stars: peculiar (except chemically peculiar)
(stars:) planetary systems
stars: Population II
stars: Population III
stars: pre-main sequence
stars: protostars
(stars:) pulsars: general
(stars:) pulsars: individual (..., ...)
stars: rotation
stars: solar-type
(stars:) starspots
stars: statistics
(stars:) subdwarfs
(stars:) supergiants
(stars:) supernovae: general
(stars:) supernovae: individual (..., ...)
stars: variables: Cepheids
stars: variables: delta Scuti
stars: variables: general
stars: variables: RR Lyrae
stars: variables: S Doradus
stars: variables: T Tauri, Herbig Ae/Be
(stars:) white dwarfs
stars: winds, outflows
stars: Wolf–Rayet

Interstellar Medium (ISM), Nebulae

ISM: abundances
ISM: atoms
ISM: bubbles
ISM: clouds
(ISM:) cosmic rays
(ISM:) dust, extinction
(ISM:) evolution
ISM: general
(ISM:) HII regions
(ISM:) Herbig–Haro objects
ISM: individual objects (..., ...) (except planetary nebulae)
ISM: jets and outflows
ISM: kinematics and dynamics
ISM: lines and bands
ISM: magnetic fields
ISM: molecules
(ISM:) planetary nebulae: general
(ISM:) planetary nebulae: individual (..., ...)
(ISM:) photon-dominated region (PDR)
ISM: structure
ISM: supernova remnants

The Galaxy

Galaxy: abundances
Galaxy: bulge
Galaxy: center
Galaxy: disk
Galaxy: evolution
Galaxy: formation
Galaxy: fundamental parameters
Galaxy: general
(Galaxy:) globular clusters: general
(Galaxy:) globular clusters: individual (..., ...)
Galaxy: halo
(Galaxy:) local interstellar matter
Galaxy: kinematics and dynamics
Galaxy: nucleus
(Galaxy:) open clusters and associations: general
(Galaxy:) open clusters and associations: individual (..., ...)
(Galaxy:) solar neighborhood
Galaxy: stellar content
Galaxy: structure


galaxies: abundances
galaxies: active
(galaxies:) BL Lacertae objects: general
(galaxies:) BL Lacertae objects: individual (..., ...)
galaxies: bulges
galaxies: clusters: general
galaxies: clusters: individual (..., ...)
galaxies: clusters: intracluster medium
galaxies: distances and redshifts
galaxies: dwarf
galaxies: elliptical and lenticular, cD
galaxies: evolution
galaxies: formation
galaxies: fundamental parameters
galaxies: general
galaxies: groups: general
galaxies: groups: individual (..., ...)
galaxies: halos
galaxies: high-redshift
galaxies: individual (..., ...)
galaxies: interactions
(galaxies:) intergalactic medium
galaxies: irregular
galaxies: ISM
galaxies: jets
galaxies: kinematics and dynamics
(galaxies:) Local Group
galaxies: luminosity function, mass function
(galaxies:) Magellanic Clouds
galaxies: magnetic fields
galaxies: nuclei
galaxies: peculiar
galaxies: photometry
(galaxies:) quasars: absorption lines
(galaxies:) quasars: emission lines
(galaxies:) quasars: general
(galaxies:) quasars: individual (..., ...)
galaxies: Seyfert
galaxies: spiral
galaxies: starburst
galaxies: star clusters: general
galaxies: star clusters: individual (..., ...)
galaxies: star formation
galaxies: statistics
galaxies: stellar content
galaxies: structure


(cosmology:) cosmic background radiation
(cosmology:) cosmological parameters
cosmology: miscellaneous
cosmology: observations
cosmology: theory
(cosmology:) dark ages, reionization, first stars
(cosmology:) dark matter
(cosmology:) dark energy
(cosmology:) diffuse radiation
(cosmology:) distance scale
(cosmology:) early universe
(cosmology:) inflation
(cosmology:) large-scale structure of universe
(cosmology:) primordial nucleosynthesis

Resolved and Unresolved Sources as a Function of Wavelength

gamma rays: diffuse background
gamma rays: galaxies
gamma rays: galaxies: clusters
gamma rays: general
gamma rays: ISM
gamma rays: stars
infrared: diffuse background
infrared: galaxies
infrared: general
infrared: ISM
infrared: planetary systems
infrared: stars
radio continuum: galaxies
radio continuum: general
radio continuum: ISM
radio continuum: planetary systems
radio continuum: stars
radio lines: galaxies
radio lines: general
radio lines: ISM
radio lines: planetary systems
radio lines: stars
submillimeter: diffuse background
submillimeter: galaxies
submillimeter: general
submillimeter: ISM
submillimeter: planetary systems
submillimeter: stars
ultraviolet: galaxies
ultraviolet: general
ultraviolet: ISM
ultraviolet: planetary systems
ultraviolet: stars
X-rays: binaries
X-rays: bursts
X-rays: diffuse background
X-rays: galaxies
X-rays: galaxies: clusters
X-rays: general
X-rays: individual (..., ...)
X-rays: ISM
X-rays: stars

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