Physics
Black Holes
100%
Magnetic Field
80%
Star Formation
48%
Neutron Stars
45%
Supernovae
40%
Angular Momentum
34%
Transients
29%
Interstellar Matter
28%
Gamma Ray Burst
28%
Anisotropy
28%
Galactic Wind
27%
Solar Wind
26%
Circumstellar Disk
26%
Stellar Feedback
25%
Supermassive Black Holes
25%
Physics
25%
Active Galactic Nuclei
24%
Star Formation Rate
22%
Galaxy Clusters
22%
Magnetohydrodynamic Simulation
22%
Dark Matter
19%
Metallicity
18%
Magnetohydrodynamics
18%
High Resolution
18%
Galactic Center
18%
Gravitational Wave
16%
Ejecta
16%
Magnetohydrodynamic Generator
16%
Massive Star
16%
Dwarf Galaxy
16%
Electromagnetic
16%
Magnetars
15%
Intracluster Medium
15%
Milky Way
15%
Heat Conduction
15%
Galactic Evolution
15%
Advection
15%
White Dwarf
14%
High Temperature Gas
14%
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%
Energetics
11%
Radiation Pressure
11%
Elliptical Galaxy
11%
Event Horizon
11%
Magnetohydrodynamic Turbulence
10%
Quasar
10%
Synchrotron
10%
Gravitational Field
9%
Galactic Nuclei
9%
Compact Objects
9%
Galaxy Masses
9%
Galaxy Halos
8%
Baryon
8%
Gravity Wave
8%
Giant Molecular Clouds
8%
Collisional Plasmas
8%
Field Strength
8%
Astrophysical Plasma
8%
Magnetic Flux
7%
Near Infrared
7%
Electron Energy
7%
High-Redshift Galaxy
7%
Distribution Function
7%
Accretion Disk
7%
Sound Wave
7%
Reionization
7%
Tidal Disruption
7%
Cooling Flow
7%
Star Cluster
6%
L Galaxies
6%
Core-Collapse Supernovae
6%
Supergiant
6%
Mass Ratio
6%
Starburst Galaxy
6%
Stellar Surfaces
6%
B Stars
6%
Mean Free Path
6%
Galactic Halos
6%
Gas Pressure
6%
Parsec
6%
Galaxy Properties
6%
Temperature Gradients
6%
Disk Galaxy
5%
Stellar Evolution
5%
Flux Density
5%
Luminosity Function
5%
Spectral Index
5%
Intergalactic Medium
5%
Radio Emission
5%
Steady State
5%
Radial-Velocity Method
5%
Globular Cluster
5%
Cyclotron Frequency
5%
Keyphrases
Galaxies
37%
Halo
25%
Turbulence
17%
Galactic Winds
17%
Star Formation
16%
Accretion Discs
14%
Accretion Flow
14%
Real Environment
14%
Cosmological Simulations
13%
Supernovae
13%
Supermassive Black Holes (SMBHs)
13%
Low-mass
13%
Solar Wind
11%
Interstellar Medium
11%
Luminosity
10%
Magnetic Field
10%
White Dwarfs
10%
Cosmic Rays
10%
Accretion Rate
10%
Alfvn Waves
10%
Sgr A*
9%
Circumgalactic Medium
9%
Stellar Feedback
9%
Shock
8%
Star Formation Rate
8%
Active Galactic nuclei
8%
Hot Gas
8%
Dwarf Galaxies
8%
Massive Black Holes
7%
Collisionality
7%
Galaxy Clusters
7%
Pressure Anisotropy
7%
Milky Way
7%
Angular Momentum
7%
Black Hole Accretion
7%
Magnetorotational Instability
7%
Hydrodynamic Simulation
6%
Eddington
6%
Dark Matter Halos
6%
Magnetohydrodynamic Simulation
6%
Galactic Center
6%
High-redshift Galaxies
6%
Stellar Masses
6%
X-ray
6%
Starburst
6%
Intracluster Medium
6%
Galactic nuclei
5%
Quasars
5%
Relativistic Magnetohydrodynamics
5%
Collision-free
5%
Galaxy Halos
5%
Globular Clusters
5%
Synchrotron
5%
Wave-driven
5%
Star-forming Galaxies
5%
Metallicity
5%
Observational Signatures
5%
Mass Loss
5%