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
|
|---|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 35
|
| Nucleosynthesis
| 26
|
| Nuclear Reactions
| 23
|
| Abundances
| 22
|
| Stars: Evolution
| 19
|
| White Dwarfs
| 14
|
| Accretion
| 14
|
| Stars: AGB And Post-AGB
| 13
|
| Supernovae: General
| 11
|
| Stars: Rotation
| 10
|
| Astrophysics
| 9
|
| Supernovae
| 9
|
| STARS: WHITE DWARFS
| 8
|
| Stars: Supernovae: General
| 8
|
| Stars: Abundances
| 8
|
| Nuclear Experiment
| 7
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 6
|
| Binaries: General
| 6
|
| Astrophysics - Astrophysics Of Galaxies
| 5
|
| Faint Blue Stars White Dwarfs Degenerate Stars Nuclei Of Planetary Nebulae
| 4
|
| Stars: Chemically Peculiar
| 4
|
| 97.20.Rp
| 4
|
| Accretion Disks
| 4
|
| Stars: Interiors
| 4
|
| 97.10.Cv
| 3
|
| Cataclysmic Variables
| 3
|
| 26.30.+k
| 3
|
| Galaxy: Abundances
| 3
|
| Nucleosynthesis In Novae Supernovae And Other Explosive Environments
| 3
|
| Stellar Structure Interiors Evolution Nucleosynthesis Ages
| 3
|
| 97.60.Bw
| 3
|
| 26.50.+x
| 2
|
| ISM: Supernova Remnants
| 2
|
| Hydrodynamics
| 2
|
| High Energy Physics - Phenomenology
| 2
|
| Globular Clusters: General
| 2
|
| Stars: Binaries
| 2
|
| Stars: Population II
| 2
|
| S Process
| 2
|
| Rotation
| 2
|
| Reaction Rate
| 2
|
| Cosmology
| 2
|
| Convection
| 2
|
| Stars: Oscillations
| 2
|
| Binaries: Close
| 2
|
| Stars: Nucleosynthesis
| 2
|
| Stars: Novae
| 2
|
| Stars: Massive
| 2
|
| Nucleosynthesis-Star: Abundances
| 2
|
| AGB Star
| 2
|
| Sun: Evolution
| 2
|
| Accretion Discs
| 2
|
| Accretion And Accretion Disks
| 2
|
| Nuclear Physics Aspects Of Novae Supernovae And Other Explosive Environments
| 2
|
| Stars: Horizontal Branch
| 2
|
| Neutrinos
| 2
|
| 97.10.Gz
| 2
|
| Isotopic Abundance
| 2
|
| Accretion: Accretion Disks
| 1
|
| Accretion Disks -Nuclear Reactions
| 1
|
| Abundances Chemical Composition
| 1
|
| 154Gd
| 1
|
| 98.80.Ft
| 1
|
| 98.58.Mj
| 1
|
| 97.30.Hk
| 1
|
| 97.20.Li
| 1
|
| 97.10.Tk
| 1
|
| 97.10.Bt
| 1
|
| 95.36.+x
| 1
|
| 28.52.-s
| 1
|
| White Dwarfs: Cooling
| 1
|
| White Dwarf
| 1
|
| The Sun [S]
| 1
|
| Supernovae: Type Ia
| 1
|
| Supernovae: Individual: Tycho
| 1
|
| Supernova Remnants
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Abundances
| 1
|
| Sun: Abundance
| 1
|
| Stellar Rotation
| 1
|
| Stellar Evolution Models
| 1
|
| Stellar Evolution
| 1
|
| Stellar Composition
| 1
|
| Stars: Wolf-Rayet
| 1
|
| Stars: Variables: Other
| 1
|
| Stars: Variables: Cepheids
| 1
|
| Stars: Population III
| 1
|
| Stars: Low-mass
| 1
|
| Stars: Individual: HD 20
| 1
|
| Stars: Early-Type
| 1
|
| Stars: Carbon
| 1
|
| Stars: Binaries: General
| 1
|
| Stars: Atmospheres
| 1
|
| Star Formation
| 1
|
| Solar System: General
| 1
|
| Short-lived Isotopes
| 1
|
| S-process
| 1
|
| Radiation Mechanisms: General
| 1
|
| Presolar Grain
| 1
|
| Physical Data And Processes
| 1
|
| Origin Formation And Abundances Of The Elements
| 1
|
| Nuclear Theory
| 1
|
| Novae
| 1
|
| Neutron Time Of Flight
| 1
|
| Neutron Spectroscopy
| 1
|
| N_TOF
| 1
|
| Line: Formation
| 1
|
| Kepler
| 1
|
| ISM: Molecules
| 1
|
| Gravitational Waves
| 1
|
| Giant And Subgiant Stars
| 1
|
| Galaxy: Halo
| 1
|
| Galaxy: Globular Clusters
| 1
|
| Galaxies: Evolution
| 1
|
| Fusion Reactors
| 1
|
| Extinction
| 1
|
| Dust
| 1
|
| Distance Scale
| 1
|
| Dissertation Summaries
| 1
|
| Dark Energy
| 1
|
| Cosmology: Cosmological Parameters
| 1
|
| Carbon Stars S Stars And Related Types
| 1
|
| Astrophysics - Galaxy Astrophysics
| 1
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 1
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 1
|
| Astroparticle Physics
| 1
|
| AGB Stars
| 1
|
| α+22Ne
| 1
|