The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
| Keyword
| Occurrences
|
|---|
| Nucleosynthesis
| 75
|
| Astrophysics
| 73
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 69
|
| STARS: EVOLUTION
| 68
|
| Nuclear Reactions
| 65
|
| Abundances
| 62
|
| Stars: Abundances
| 49
|
| Stars: AGB And Post-AGB
| 47
|
| Nuclear Experiment
| 37
|
| Stars: Interiors
| 25
|
| Stars: Carbon
| 23
|
| Stellar Evolution
| 21
|
| Stars: Population II
| 16
|
| 97.10.Cv
| 12
|
| Stellar Structure Interiors Evolution Nucleosynthesis Ages
| 12
|
| Stars: White Dwarfs
| 11
|
| Stellar Models
| 10
|
| Globular Clusters
| 9
|
| Supernovae
| 9
|
| Hydrostatic Stellar Nucleosynthesis
| 9
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 9
|
| Solar Neutrinos
| 9
|
| Metallicity
| 9
|
| Stars: AGB
| 9
|
| Stellar Hydrogen Burning
| 9
|
| Mass Function
| 9
|
| 25.40.Lw
| 9
|
| STARS: LUMINOSITY FUNCTION
| 9
|
| Radiative Capture
| 9
|
| 26.20.Cd
| 8
|
| Abundances Chemical Composition
| 8
|
| Big Bang Nucleosynthesis
| 8
|
| 97.20.Li
| 8
|
| Giant And Subgiant Stars
| 8
|
| Stars: Late-type
| 8
|
| 97.10.Tk
| 8
|
| 26.20.+f
| 8
|
| 26.65.+t
| 8
|
| High Energy Physics - Phenomenology
| 8
|
| AGB Stars
| 7
|
| 26.35.+c
| 7
|
| Stars: Rotation
| 7
|
| Supernovae: General
| 7
|
| GALAXY: GLOBULAR CLUSTERS: GENERAL
| 7
|
| Stars: Nucleosynthesis
| 6
|
| Stars: Supernovae: General
| 6
|
| Nuclear Astrophysics
| 6
|
| Stars: Low-mass
| 6
|
| White Dwarfs
| 6
|
| 3H- 3He- And 4He-induced Reactions
| 6
|
| 25.55.-e
| 6
|
| Stellar Interiors
| 5
|
| Nucleosynthesis In Novae Supernovae And Other Explosive Environments
| 5
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 5
|
| Helium
| 5
|
| Hertzsprung-Russell Diagram
| 5
|
| Stellar Mass
| 5
|
| Color-Magnitude Diagram
| 5
|
| Astrophysics - Astrophysics Of Galaxies
| 5
|
| 97.20.Tr
| 4
|
| Convection
| 4
|
| Brown Dwarfs
| 4
|
| 97.20.Rp
| 4
|
| Main Sequence Stars
| 4
|
| Faint Blue Stars White Dwarfs Degenerate Stars Nuclei Of Planetary Nebulae
| 4
|
| Accretion
| 4
|
| Cosmology: Cosmological Parameters
| 4
|
| Abundance
| 4
|
| 26.20.+f Hydrostatic Stellar Nucleosynthesis
| 4
|
| Globular Clusters: General
| 4
|
| Stellar Luminosity
| 4
|
| S-process
| 4
|
| Stellar Composition
| 4
|
| Hydrogen
| 4
|
| 25.40.Lw Radiative Capture
| 4
|
| Stars: Chemically Peculiar
| 4
|
| Population II Stars
| 4
|
| Star Clusters
| 3
|
| Techniques: Spectroscopic
| 3
|
| Stars: Oscillations
| 3
|
| Red Giant Stars
| 3
|
| Cosmology
| 3
|
| CLUSTERS: GLOBULAR
| 3
|
| Carbon Stars S Stars And Related Types
| 3
|
| Carbon Stars
| 3
|
| Physics - Instrumentation And Detectors
| 3
|
| Asymptotic Giant Branch Stars
| 3
|
| Origin Formation And Abundances Of The Elements
| 3
|
| Inelastic Proton Scattering
| 3
|
| High Energy Physics - Experiment
| 3
|
| Opacity
| 3
|
| 98.80.Ft
| 3
|
| 97.60.Bw
| 3
|
| Stars: Atmospheres
| 3
|
| 97.30.Hk
| 3
|
| Nuclear Physics Aspects Of Novae Supernovae And Other Explosive Environments
| 3
|
| Nuclear Fusion
| 3
|
| Galaxy: Globular Clusters: Individual: Name: ω Centauri
| 3
|
| 26.50.+x
| 3
|
| 26.30.-k
| 3
|
| Stars: Variables: General
| 3
|
| 25.40.Ep
| 3
|
| 26.30.+k
| 2
|
| Population III Stars
| 2
|
| Charge Coupled Devices
| 2
|
| Nuclear Theory
| 2
|
| Stars: C And S Rich
| 2
|
| Late Stellar Evolution
| 2
|
| 98.20.Gm
| 2
|
| Stars: Binaries
| 2
|
| GALAXY: GLOBULAR CLUSTERS
| 2
|
| Globular Clusters In The Milky Way
| 2
|
| Galactic Evolution
| 2
|
| Star Formation
| 2
|
| Collective
| 2
|
| Computational Astrophysics
| 2
|
| Cosmology: Distance Scale
| 2
|
| Stars: Low Mass
| 2
|
| Stars: Mass Loss
| 2
|
| Diffusion
| 2
|
| Thermonuclear Reactions
| 2
|
| GALAXIES: EVOLUTION
| 2
|
| Galaxies: Local Group
| 2
|
| Distance Scale
| 2
|
| Magellanic Clouds
| 2
|
| 97.10.Bt
| 2
|
| Dwarf Galaxies
| 2
|
| Masses
| 2
|
| ELEMENTARY PARTICLES
| 2
|
| GALAXY: OPEN CLUSTERS AND ASSOCIATIONS: GENERAL
| 2
|
| Stellar Structure
| 2
|
| 29.30.Kv X- And γ-ray Spectroscopy
| 2
|
| 29.30.Kv
| 2
|
| 29.17.+w Electrostatic
| 2
|
| Techniques: Photometric
| 2
|
| Underground Nuclear Physics
| 2
|
| GALAXY: GLOBULAR CLUSTERS: INDIVIDUAL: MESSIER NUMBER: M3
| 2
|
| Experimental Nuclear Astrophysics
| 2
|
| Extinction
| 2
|
| GALAXIES: STAR CLUSTERS
| 2
|
| Galactic Clusters
| 2
|
| Hydrodynamics
| 2
|
| Galaxy: Abundances
| 2
|
| Stellar Abundances
| 2
|
| Hydrogen Burning
| 2
|
| Open Clusters
| 2
|
| The Sun [S]
| 2
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| STARS: HORIZONTAL-BRANCH
| 2
|
| Stellar Convection
| 2
|
| White Dwarf
| 2
|
| Tables (Data)
| 2
|
| GLOBULAR CLUSTERS: INDIVIDUAL (ω CENTAURI)
| 1
|
| Globular Clusters: Age
| 1
|
| Globular Clusters In External Galaxies
| 1
|
| Giant Stars
| 1
|
| Germanium Detector
| 1
|
| General
| 1
|
| GEANT4 Simulation
| 1
|
| Gamma-ray Total Absorption Spectroscopy
| 1
|
| Gamma Transitions And Level Energies
| 1
|
| Gamma Spectroscopy
| 1
|
| GALAXY: HALO
| 1
|
| Galaxy: Globular Clusters: NGC 6397
| 1
|
| GALAXY: FUNDAMENTAL PARAMETERS
| 1
|
| Galaxy: Formation
| 1
|
| Galaxy: Evolution
| 1
|
| GALAXIES: MAGELLANIC CLOUDS
| 1
|
| Galaxies: Intergalactic Medium
| 1
|
| Galaxies: Individual: LMC SMC Carina
| 1
|
| Galaxies: Individual (LMC)
| 1
|
| Galaxies: Formation
| 1
|
| Galaxies: Abundances
| 1
|
| Galaxies
| 1
|
| Fusion Reactors
| 1
|
| Fission Reactors
| 1
|
| Equations Of State
| 1
|
| Energetic Neutron
| 1
|
| Ellipsoidal Variable Stars
| 1
|
| Element Abundances
| 1
|
| Electrostatic Collective And Linear Accelerators
| 1
|
| Electron-Positron Pairs
| 1
|
| Dwarfs
| 1
|
| Dwarf Spheroidal Galaxies
| 1
|
| Dust
| 1
|
| Distances Redshifts Radial Velocities
| 1
|
| Distance
| 1
|
| Direct Reactions
| 1
|
| Direct Cross-section
| 1
|
| Deuterium
| 1
|
| Dark Energy
| 1
|
| Coulomb Collisions
| 1
|
| Cosmology: Theory
| 1
|
| Cosmology: Observations
| 1
|
| Cosmogony
| 1
|
| Compton Continuum
| 1
|
| Chemical Evolution
| 1
|
| Chemical Composition And Chemical Evolution
| 1
|
| Cataclysmic Variables
| 1
|
| Carbon 13
| 1
|
| Camera: Antarctic Infrared
| 1
|
| Calibrating
| 1
|
| C-M Diagrams
| 1
|
| Binary Stars
| 1
|
| Binary And Multiple Stars
| 1
|
| Binaries: Close
| 1
|
| Big Bang Cosmology
| 1
|
| Baryons
| 1
|
| Asymptotic Giant Branch
| 1
|
| Astroparticles: Axions
| 1
|
| Astroparticle Physics
| 1
|
| Astronomy
| 1
|
| Astronomical Photometry
| 1
|
| Astrometry
| 1
|
| Antarctica
| 1
|
| Antarctic Permanent Observatories
| 1
|
| Antarctic Astronomy
| 1
|
| And Linear Accelerators
| 1
|
| AGB Stars: Nucleosynthesis
| 1
|
| AGB Nucleosynthesis
| 1
|
| AGB
| 1
|
| Activation Measurement
| 1
|
| Accretion: Accretion Disks
| 1
|
| Accretion Disks
| 1
|
| Accretion And Accretion Disks
| 1
|
| Abundances - Stars: AGB And Post-AGB
| 1
|
| 99.10.Fg
| 1
|
| 98.62.Py
| 1
|
| 98.62.Bj
| 1
|
| 98.58.Mj
| 1
|
| 98.52.Wz
| 1
|
| 98.38.Ly
| 1
|
| 98.20.Jp
| 1
|
| 97.80.-d
| 1
|
| 97.60.-s
| 1
|
| 97.30.Qt
| 1
|
| 97.10.Zr
| 1
|
| 97.10.Yp
| 1
|
| 97.10.Nf
| 1
|
| 97.10.Me
| 1
|
| 97.10.Gz
| 1
|
| 97.10.Ex
| 1
|
| 96.10.+i
| 1
|
| 95.75.Fg
| 1
|
| 95.36.+x
| 1
|
| 6Li Abundance
| 1
|
| 34.50.Bw Energy Loss And Stopping Power
| 1
|
| 29.17.+w
| 1
|
| 28.52.-s
| 1
|
| 28.41.-i
| 1
|
| 26.65.+t Solar Neutrinos
| 1
|
| 26.20.Fj
| 1
|
| 26.20.+f Hydrostatic Steller Nucleosynthesis
| 1
|
| 25.60.Dz Interaction And Reaction Cross Sections
| 1
|
| (stars:) Binaries: Eclipsing
| 1
|
| X-ray Binary Stars
| 1
|
| X- And γ-ray Spectroscopy
| 1
|
| X- And Gamma-ray Spectroscopy
| 1
|
| White Dwarfs: Cooling
| 1
|
| Underground Physics
| 1
|
| Underground Laboratory
| 1
|
| Underground
| 1
|
| Time
| 1
|
| Thermodynamic Properties
| 1
|
| Telescopes: Robotic
| 1
|
| Telescopes
| 1
|
| Target Chamber
| 1
|
| Symbiotic Binary Stars
| 1
|
| Supernovae: Type Ia
| 1
|
| Supernovae: Stellar Evolution
| 1
|
| Supernovae: Progenitors
| 1
|
| Supernovae: Individual: Tycho
| 1
|
| Supernova Remnants
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Evolution
| 1
|
| Sun: Abundance
| 1
|
| Subdwarf Stars
| 1
|
| Sub-stellar Objects
| 1
|
| Stellar Spectrophotometry
| 1
|
| Stellar Populations: Galaxy
| 1
|
| Stellar Populations: Galaxies
| 1
|
| Stellar Physics
| 1
|
| Stellar Nucleosynthesis
| 1
|
| Stellar Model
| 1
|
| Stellar Helium Burning
| 1
|
| Stellar Evolution Models
| 1
|
| Stellar Color
| 1
|
| Stellar Atmospheres
| 1
|
| Stars: Wolf-Rayet
| 1
|
| Stars: White Dwarf
| 1
|
| Stars: Variables: Cepheids
| 1
|
| Stars: Supernovae
| 1
|
| Stars: Structure
| 1
|
| Stars: Starspots
| 1
|
| Stars: Population III
| 1
|
| Stars: Mixing
| 1
|
| Stars: Metal Poor
| 1
|
| Stars: Massive
| 1
|
| Stars: Individual: V841 Centauri
| 1
|
| Stars: Individual: V1034 Centauri
| 1
|
| STARS: INDIVIDUAL: IRC+10216
| 1
|
| Stars: Individual: IRAS 08143-4406
| 1
|
| Stars: Individual: IRAS 06530-0213
| 1
|
| Stars: Individual: HE 1305+0132
| 1
|
| STARS: HR DIAGRAM
| 1
|
| Stars: Horizontal Branch
| 1
|
| Stars: Fundamental Parameters
| 1
|
| STARS: COLOR-MAGNITUDE DIAGRAMS
| 1
|
| STARS: CIRCUMSTELLAR MATTER
| 1
|
| Stars: C Ans S Rich
| 1
|
| Stars: AGB And Post-AGB - Stars: Low-mass
| 1
|
| Stars: AGB And
| 1
|
| Stars: Activity
| 1
|
| Star Counts Distribution And Statistics
| 1
|
| Spectroscopy And Spectrophotometry
| 1
|
| Spatial Distribution Of Galaxies
| 1
|
| Solar System: General
| 1
|
| Solar Nebula
| 1
|
| Site Testing
| 1
|
| Short-lived Isotopes
| 1
|
| Semi-regular Variable Stars
| 1
|
| Segmented Bismuth Germanium Oxide (BGO) Detector
| 1
|
| Rotation
| 1
|
| Resonance Reactions
| 1
|
| Ratios
| 1
|
| RADIO LINES: STARS
| 1
|
| Radii
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiative Heat Transfer
| 1
|
| Radiation Shielding And Background Reduction
| 1
|
| Publisher's Note
| 1
|
| Primordial Stars
| 1
|
| Primordial Nucleosynthesis
| 1
|
| Presolar Grains
| 1
|
| Post-AGB
| 1
|
| POP. III
| 1
|
| Planetary Nebulae
| 1
|
| Physics
| 1
|
| Photons
| 1
|
| PACS:26.20.+f Hydrostatic Stellar Nucleosynthesis – 25.60.Dz Interaction And Reaction Cross Sections
| 1
|
| PACS:26.20.+f Hydrostatic Stellar Nucleosynthesis &ndash
| 1
|
| PACS. 26.20.+f Hydrostatic Stellar Nucleosynthesis – 34.50.-s Scattering Of Atoms And Nucleus
| 1
|
| OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL
| 1
|
| Opacity And Line Formation
| 1
|
| Numerical Analysis
| 1
|
| Nucleosynthesis: Stellar Evolution
| 1
|
| Nucleosynthesis: Light Elements
| 1
|
| Nucleosynthesis: AGB Stars
| 1
|
| Nuclear Reactions: Stellar Evolution
| 1
|
| Nuclear Reactions: Cross Sections
| 1
|
| Nuclear Reactions: Astrophysics
| 1
|
| Nuclear Astrophysics Experiment
| 1
|
| Novae Dwarf Novae Recurrent Novae And Other Cataclysmic Variables
| 1
|
| Novae
| 1
|
| NGC 7789
| 1
|
| Neutron Stars
| 1
|
| Neutron Irradiation
| 1
|
| Neutron
| 1
|
| Neutrinos
| 1
|
| Multiple Star Evolution
| 1
|
| Milky Way Galaxy
| 1
|
| Mid-infrared
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical
| 1
|
| Meteorites: Nucleosynthesis
| 1
|
| Metallic Stars
| 1
|
| Metal-Poor Stars
| 1
|
| Mathematical Models
| 1
|
| Massive Stars
| 1
|
| Mass Loss And Stellar Winds
| 1
|
| Mass
| 1
|
| Magnetic Fields
| 1
|
| LUNA
| 1
|
| Luminosity
| 1
|
| Low-mass X-ray Binary Stars
| 1
|
| Low-background
| 1
|
| Long Period Variable Stars
| 1
|
| Lithium Problem
| 1
|
| Linear Accelerators
| 1
|
| Line: Identification
| 1
|
| Lead Stars
| 1
|
| Late-type Supergiant Stars
| 1
|
| Late Stages Of Stellar Evolution
| 1
|
| Krypton
| 1
|
| Keywords: Nuclear Reactions
| 1
|
| Kepler
| 1
|
| Isotopic Abundances
| 1
|
| ISM: Supernova Remnants
| 1
|
| ISM: Dust
| 1
|
| ISM: Abundances
| 1
|
| Ionization
| 1
|
| Interstellar Extinction
| 1
|
| Instrumentation: Miscellaneous
| 1
|
| INSTABILITIES [H]
| 1
|
| Infrared: Survey
| 1
|
| Infrared: Instrumentation
| 1
|
| Infrared Photometry
| 1
|
| Ideal Gas
| 1
|
| High Resolution Spectroscopy
| 1
|
| Hertzsprung-Russell Color-magnitude And Color-color Diagrams
| 1
|
| Hertzsprung-Russell
| 1
|
| Helium-3 Counter
| 1
|
| Helium Isotopes
| 1
|
| H Burning Stars He Burning Stars
| 1
|
| GLOBULAR CLUSTERS: INDIVIDUAL: NGC 6366
| 1
|
| Globular Clusters: Individual: NGC 1866
| 1
|
| Globular Clusters: Individual: M4
| 1
|
| 24.50.+g
| 1
|
| 24.30.-v
| 1
|
| 23.20.Lv
| 1
|
| 14.80.Va
| 1
|
| (stars:) White Dwarfs
| 1
|
| (stars:) Binaries: Symbiotic
| 1
|
| (stars:) Binaries: General
| 1
|
| {s
| 1
|