Physics
Active Galactic Nuclei
29%
Anisotropy
13%
Baryon
20%
Cosmic Microwave Background
10%
Dark Matter
24%
Density Distribution
22%
Distribution Function
63%
Early Star
7%
Early Universe
7%
Faraday Effect
9%
Galactic Evolution
8%
Giant Molecular Clouds
8%
Globular Cluster
16%
High Resolution
21%
Initial Mass Function
11%
Intergalactic Medium
11%
Interstellar Matter
79%
Interstellar Synchrotron Emission
13%
Kinetic Energy
8%
Line of Sight
16%
Linear Polarization
7%
Linewidth
9%
Luminosity Function
11%
Mach Number
85%
Machine Learning
17%
Magnetic Field
59%
Magnetohydrodynamic Generator
18%
Magnetohydrodynamic Simulation
15%
Magnetohydrodynamic Turbulence
51%
Magnetohydrodynamics
8%
Massive Star
7%
Milky Way
9%
Molecular Clouds
57%
Molecular Gas
10%
Physics
12%
Power Spectra
39%
Radiative Transfer
15%
Small Magellanic Cloud
12%
Southern Sky
7%
Star Cluster
9%
Star Formation
100%
Star Formation Rate
34%
Stellar Feedback
23%
Stellar Mass Functions
8%
Superbubbles
12%
Supernovae
28%
Supersonics
63%
Synchrotron
15%
Transonic Flow
8%
Turbulent Medium
22%
Keyphrases
Arecibo
5%
Astrophysics
6%
Baryons
11%
Bursting Bubble
10%
Column Density
17%
Dark Matter
16%
Dark Matter Halos
7%
Decorrelation Scales
6%
Density Fluctuations
7%
Density Probability
9%
Density Structure
5%
Formation Quality
8%
Galactic
5%
Galactic Outflows
6%
Galaxies
29%
Gas Density
6%
Giant Molecular Clouds
5%
Globular Clusters
13%
High-redshift Galaxies
6%
Initial Mass Function
11%
Interstellar Medium
34%
Interstellar Turbulence
17%
James Webb Space Telescope
6%
Line-of-sight
10%
Luminosity Function
5%
Mach number
24%
Magnetic Field
19%
Magnetohydrodynamic (MHD) Turbulence
17%
Molecular Clouds
17%
Molecular Gas
11%
Nebulae
5%
Number Relations
6%
Numerical Simulation
5%
Polarization Gradient
10%
Probability Distribution Function
13%
Radio
10%
Spatially Resolved
6%
Star Clusters
10%
Star Formation
40%
Star Formation Rate
17%
Star-forming
10%
Stellar Feedback
8%
Streamwise Velocity
6%
Superbubbles
12%
Supernovae
18%
Surface Density
8%
Synchrotron
10%
Turbulence
42%
Turbulent Media
15%
Velocity Dispersion
7%