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 - Astrophysics Of Galaxies
| 91
|
| Magnetohydrodynamics [S]
| 36
|
| Turbulence
| 31
|
| ISM: Structure
| 23
|
| Interstellar Medium
| 16
|
| Star Formation
| 15
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 13
|
| ISM: Clouds
| 12
|
| Stars: Formation
| 11
|
| Galaxies: Star Formation
| 10
|
| ISM: Kinematics And Dynamics
| 9
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 8
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 8
|
| ISM: Magnetic Fields
| 7
|
| Methods: Numerical
| 7
|
| ISM: General
| 6
|
| Galaxy Formation
| 6
|
| Polarization
| 6
|
| Cosmology
| 6
|
| Stellar Feedback
| 5
|
| Galaxies: Evolution
| 5
|
| Galaxies: Formation
| 5
|
| Galaxies: ISM
| 5
|
| High-redshift Galaxies
| 4
|
| Molecular Clouds
| 4
|
| Giant Molecular Clouds
| 4
|
| Extinction
| 4
|
| Dust
| 4
|
| Methods: Data Analysis
| 4
|
| Intergalactic Medium
| 4
|
| Magnetic Fields
| 4
|
| Hydrodynamical Simulations
| 4
|
| Intergalactic Gas
| 3
|
| Radiative Transfer [S]
| 3
|
| Magnetohydrodynamical Simulations
| 3
|
| Protostars
| 3
|
| Lyman Alpha Forest
| 3
|
| Extragalactic Astronomy
| 3
|
| Plasma Astrophysics
| 3
|
| Computational Methods
| 3
|
| Photon-dominated Region: PDR
| 3
|
| Astrostatistics
| 3
|
| Interstellar Magnetic Fields
| 3
|
| Supernova Remnants
| 3
|
| Physics - Fluid Dynamics
| 3
|
| Cosmology: Theory
| 2
|
| Galaxies: High-redshift
| 2
|
| Galaxy Evolution
| 2
|
| Starburst Galaxies
| 2
|
| Star Forming Regions
| 2
|
| Massive Stars
| 2
|
| Physics - Space Physics [H]
| 2
|
| Photodissociation Regions
| 2
|
| Shocks
| 2
|
| Astronomy Databases
| 2
|
| Radio Lines: ISM
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Interstellar Molecules
| 2
|
| Radio Continuum: ISM
| 2
|
| Radio Astronomy
| 2
|
| Globular Star Clusters
| 2
|
| Molecular Data
| 2
|
| Astrophysical Fluid Dynamics
| 2
|
| Astrophysics - Earth And Planetary Astrophysics
| 2
|
| Galactic And Extragalactic Astronomy
| 2
|
| James Webb Space Telescope
| 2
|
| Dwarf Galaxies
| 2
|
| Polarimetry
| 2
|
| Active Galactic Nuclei
| 2
|
| Initial Mass Function
| 2
|
| Magellanic Clouds
| 2
|
| Galactic Magnetic Fields
| 1
|
| Galactic Cosmic Rays
| 1
|
| Early Universe
| 1
|
| Disk Galaxies
| 1
|
| Diffuse Radiation
| 1
|
| Cosmological Parameters From Large-scale Structure
| 1
|
| Cosmic Microwave Background Radiation
| 1
|
| Cosmic Background Radiation
| 1
|
| Convolutional Neural Networks
| 1
|
| Computer Science - Machine Learning
| 1
|
| Computer Science - Artificial Intelligence
| 1
|
| CO Line Emission
| 1
|
| Circumgalactic Medium
| 1
|
| Chemical Abundances
| 1
|
| B Stars
| 1
|
| Astrostatistics Techniques
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astrophysics - Galaxy Astrophysics
| 1
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 1
|
| Astrophysics
| 1
|
| Astrophysical Black Holes
| 1
|
| Young Stellar Objects
| 1
|
| Young Star Clusters
| 1
|
| Waves
| 1
|
| Ultraviolet Spectroscopy
| 1
|
| Ultraviolet Astronomy
| 1
|
| Theoretical Models
| 1
|
| Telescopes
| 1
|
| Techniques: Polarimetric
| 1
|
| Supermassive Black Holes
| 1
|
| Superbubbles
| 1
|
| Submillimetre: ISM
| 1
|
| Stellar Wind Bubbles
| 1
|
| Stellar Jets
| 1
|
| Stars: Winds
| 1
|
| Stars: Low-mass
| 1
|
| Starlight Polarization
| 1
|
| Star Clusters
| 1
|
| Spectroscopy
| 1
|
| Space Vehicles
| 1
|
| Shock Waves
| 1
|
| Rosette
| 1
|
| Radio Observatories
| 1
|
| Radio Lines: General
| 1
|
| Radio Interferometers
| 1
|
| Radio Continuum: Galaxies
| 1
|
| Radiative Transfer Simulations
| 1
|
| Radiative Processes
| 1
|
| Primordial Galaxies
| 1
|
| Planet–star Interactions
| 1
|
| Planets And Satellites: Magnetic Fields
| 1
|
| Physics - Computational Physics
| 1
|
| Outflows
| 1
|
| Oort Cloud Objects
| 1
|
| Non-Gaussianity
| 1
|
| Molecular Gas
| 1
|
| Millimeter Astronomy
| 1
|
| MHD (magnetohydrodynamics)
| 1
|
| Methods:statistical Numerical
| 1
|
| Methods: Statistical
| 1
|
| Magneto-hydrodynamics Simulations
| 1
|
| Luminosity Function
| 1
|
| Local Group
| 1
|
| Large-scale Structure Of Universe
| 1
|
| ISM: Molecules
| 1
|
| ISM: Jets And Outflows
| 1
|
| ISM: Individual Objects: Orion A
| 1
|
| ISM: Evolution
| 1
|
| ISM: Abundances
| 1
|
| Interstellar Synchrotron Emission
| 1
|
| Interstellar Plasma
| 1
|
| Interstellar Dynamics
| 1
|
| Interstellar Dust Extinction
| 1
|
| Interstellar Dust
| 1
|
| Interstellar Atomic Gas
| 1
|
| Interplanetary Medium [H]
| 1
|
| Hydrodynamics
| 1
|
| H I Line Emission
| 1
|
| Gas-to-dust Ratio
| 1
|
| Gamma-rays
| 1
|
| Galaxy: Halo
| 1
|
| Galaxy Rotation Curves
| 1
|
| Galaxy Processes
| 1
|
| Galaxy Physics
| 1
|
| Galaxy Mergers
| 1
|
| Galaxy Dynamics
| 1
|
| Galaxy Dark Matter Halos
| 1
|
| Galaxies: Structure
| 1
|
| Galaxies: Starburst
| 1
|
| Galaxies: Dwarf
| 1
|
| Galaxies: Clusters: Individual: Virgo
| 1
|
| Galaxies
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomical Simulations
| 1
|
| Astrochemistry
| 1
|
| Analytical Mathematics
| 1
|
| Galactic Winds
| 1
|