Physics
Black Holes
100%
Magnetic Field
82%
Star Formation
48%
Neutron Stars
45%
Supernovae
40%
Angular Momentum
35%
Transients
29%
Supermassive Black Holes
29%
Interstellar Matter
28%
Gamma Ray Burst
28%
Anisotropy
28%
Galactic Wind
27%
Solar Wind
26%
Circumstellar Disk
26%
Stellar Feedback
25%
Physics
25%
Active Galactic Nuclei
24%
Magnetohydrodynamic Simulation
24%
Star Formation Rate
22%
Galaxy Clusters
22%
Dark Matter
19%
Metallicity
18%
Magnetohydrodynamics
18%
Galactic Center
18%
High Resolution
18%
Gravitational Wave
18%
Ejecta
16%
Magnetohydrodynamic Generator
16%
Massive Star
16%
Electromagnetic
16%
Dwarf Galaxy
16%
Magnetars
15%
Intracluster Medium
15%
Milky Way
15%
Heat Conduction
15%
Galactic Evolution
15%
Advection
15%
High Temperature Gas
15%
White Dwarf
15%
Milky Way Mass
13%
Light Curve
13%
Stellar Mass
13%
Interstellar Synchrotron Emission
12%
Stellar Wind
12%
Collisionless Plasmas
12%
Circumstellar Disks
12%
Thermal Instability
11%
Event Horizon
11%
Energetics
11%
Radiation Pressure
11%
Elliptical Galaxy
11%
Quasar
10%
Magnetohydrodynamic Turbulence
10%
Synchrotron
10%
Gravitational Field
9%
Galactic Nuclei
9%
Compact Objects
9%
Galaxy Masses
9%
Galaxy Halos
8%
Magnetic Flux
8%
Baryon
8%
Gravity Wave
8%
Tidal Disruption
8%
Giant Molecular Clouds
8%
Collisional Plasmas
8%
Field Strength
8%
Astrophysical Plasma
8%
Near Infrared
7%
Electron Energy
7%
High-Redshift Galaxy
7%
Distribution Function
7%
Accretion Disk
7%
Sound Wave
7%
Reionization
7%
Cooling Flow
7%
Stellar Surfaces
6%
Star Cluster
6%
L Galaxies
6%
Core-Collapse Supernovae
6%
Supergiant
6%
Mass Ratio
6%
Starburst Galaxy
6%
B Stars
6%
Mean Free Path
6%
Galactic Halos
6%
Gas Pressure
6%
Parsec
6%
Galaxy Properties
6%
Temperature Gradients
6%
Luminosity Function
5%
Disk Galaxy
5%
Stellar Evolution
5%
Flux Density
5%
Spectral Index
5%
Radio Emission
5%
Intergalactic Medium
5%
Steady State
5%
Radial-Velocity Method
5%
Globular Cluster
5%
Cyclotron Frequency
5%
Keyphrases
Galaxies
38%
Halo
25%
Turbulence
17%
Galactic Winds
17%
Star Formation
16%
Supermassive Black Holes (SMBHs)
15%
Accretion Flow
15%
Cosmological Simulations
15%
Accretion Discs
15%
Real Environment
14%
Supernovae
14%
Low-mass
13%
Luminosity
12%
Accretion Rate
12%
Magnetic Field
11%
Solar Wind
11%
Interstellar Medium
11%
White Dwarfs
10%
Cosmic Rays
10%
Alfvn Waves
10%
Shock
10%
Sgr A*
9%
Circumgalactic Medium
9%
Stellar Feedback
9%
Hot Gas
8%
Milky Way
8%
Angular Momentum
8%
Dwarf Galaxies
8%
Star Formation Rate
8%
Active Galactic nuclei
8%
Massive Black Holes
7%
Magnetohydrodynamic Simulation
7%
Collisionality
7%
Galaxy Clusters
7%
Pressure Anisotropy
7%
Hydrodynamic Simulation
7%
Black Hole Accretion
7%
Magnetorotational Instability
7%
Galactic Center
6%
Eddington
6%
Synchrotron
6%
Dark Matter Halos
6%
Relativistic Magnetohydrodynamics
6%
High-redshift Galaxies
6%
Stellar Masses
6%
X-ray
6%
Starburst
6%
Elliptical Galaxies
6%
Intracluster Medium
6%
Galactic nuclei
5%
Quasars
5%
Galaxy Halos
5%
Collision-free
5%
Metallicity
5%
Globular Clusters
5%
Mass Loss
5%
Wave-driven
5%
Star-forming Galaxies
5%
Observational Signatures
5%
