Physics
Accretion Disk
7%
Active Galactic Nuclei
24%
Advection
15%
Angular Momentum
34%
Anisotropy
28%
Astrophysical Plasma
8%
B Stars
6%
Baryon
8%
Black Holes
100%
Circumstellar Disk
26%
Circumstellar Disks
12%
Collisional Plasmas
8%
Collisionless Plasmas
12%
Compact Objects
9%
Cooling Flow
7%
Core-Collapse Supernovae
6%
Cyclotron Frequency
5%
Dark Matter
19%
Disk Galaxy
5%
Distribution Function
7%
Dwarf Galaxy
16%
Ejecta
16%
Electromagnetic
16%
Electron Energy
7%
Elliptical Galaxy
11%
Energetics
11%
Event Horizon
11%
Field Strength
8%
Flux Density
5%
Galactic Center
18%
Galactic Evolution
15%
Galactic Halos
6%
Galactic Nuclei
9%
Galactic Wind
27%
Galaxy Clusters
22%
Galaxy Halos
8%
Galaxy Masses
9%
Galaxy Properties
6%
Gamma Ray Burst
28%
Gas Pressure
6%
Giant Molecular Clouds
8%
Globular Cluster
5%
Gravitational Field
9%
Gravitational Wave
16%
Gravity Wave
8%
Heat Conduction
15%
High Resolution
18%
High Temperature Gas
14%
High-Redshift Galaxy
7%
Intergalactic Medium
5%
Interstellar Matter
28%
Interstellar Synchrotron Emission
12%
Intracluster Medium
15%
L Galaxies
6%
Light Curve
13%
Luminosity Function
5%
Magnetars
15%
Magnetic Field
80%
Magnetic Flux
7%
Magnetohydrodynamic Generator
16%
Magnetohydrodynamic Simulation
22%
Magnetohydrodynamic Turbulence
10%
Magnetohydrodynamics
18%
Mass Ratio
6%
Massive Star
16%
Mean Free Path
6%
Metallicity
18%
Milky Way
15%
Milky Way Mass
13%
Near Infrared
7%
Neutron Stars
45%
Parsec
6%
Physics
25%
Quasar
10%
Radial-Velocity Method
5%
Radiation Pressure
11%
Radio Emission
5%
Reionization
7%
Solar Wind
26%
Sound Wave
7%
Spectral Index
5%
Star Cluster
6%
Star Formation
48%
Star Formation Rate
22%
Starburst Galaxy
6%
Steady State
5%
Stellar Evolution
5%
Stellar Feedback
25%
Stellar Mass
13%
Stellar Surfaces
6%
Stellar Wind
12%
Supergiant
6%
Supermassive Black Holes
25%
Supernovae
40%
Synchrotron
10%
Temperature Gradients
6%
Thermal Instability
11%
Tidal Disruption
7%
Transients
29%
White Dwarf
14%
Keyphrases
Accretion Discs
14%
Accretion Flow
14%
Accretion Rate
10%
Active Galactic nuclei
8%
Alfvn Waves
10%
Angular Momentum
7%
Black Hole Accretion
7%
Circumgalactic Medium
9%
Collision-free
5%
Collisionality
7%
Cosmic Rays
10%
Cosmological Simulations
13%
Dark Matter Halos
6%
Dwarf Galaxies
8%
Eddington
6%
Galactic Center
6%
Galactic nuclei
5%
Galactic Winds
17%
Galaxies
37%
Galaxy Clusters
7%
Galaxy Halos
5%
Globular Clusters
5%
Halo
25%
High-redshift Galaxies
6%
Hot Gas
8%
Hydrodynamic Simulation
6%
Interstellar Medium
11%
Intracluster Medium
6%
Low-mass
13%
Luminosity
10%
Magnetic Field
10%
Magnetohydrodynamic Simulation
6%
Magnetorotational Instability
7%
Mass Loss
5%
Massive Black Holes
7%
Metallicity
5%
Milky Way
7%
Observational Signatures
5%
Pressure Anisotropy
7%
Quasars
5%
Real Environment
14%
Relativistic Magnetohydrodynamics
5%
Sgr A*
9%
Shock
8%
Solar Wind
11%
Star Formation
16%
Star Formation Rate
8%
Star-forming Galaxies
5%
Starburst
6%
Stellar Feedback
9%
Stellar Masses
6%
Supermassive Black Holes (SMBHs)
13%
Supernovae
13%
Synchrotron
5%
Turbulence
17%
Wave-driven
5%
White Dwarfs
10%
X-ray
6%
