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Physics
Star Formation
100%
Protostars
55%
Molecular Clouds
36%
High-Mass Stars
34%
Star Forming Regions
31%
Magnetic Field
29%
Massive Star
23%
Young Stellar Objects
22%
Spectral Energy Distribution
21%
Gould Belt
20%
Hydroxyl Masers
19%
Linewidth
17%
Infrared Dark Clouds
17%
Radiative Transfer
15%
Low Noise
14%
Star Formation Rate
12%
Flux Density
11%
Circumstellar Disks
11%
Dark Interstellar Clouds
11%
Near Infrared
11%
Spectral Index
11%
Galactic Longitude
10%
Vapor Phase
9%
Kinetic Energy
9%
Point Source
9%
Spiral Arms
9%
Protoclusters
9%
Milky Way
9%
Stellar Wind
8%
Low-Mass Star
8%
Line of Sight
8%
T Tauri Stars
7%
Line Spectra
7%
Magellanic Clouds
7%
Bolometer
7%
Field Strength
7%
High Resolution
7%
Very Large Array
7%
Millimeter Astronomy
6%
Gravitational Energy
6%
Water Maser
6%
Emissivity
6%
Dust Continuum Emission
6%
Parsec
6%
Energetics
6%
Radio Astronomy
5%
Planetary Nebula
5%
Chemical Evolution
5%
Radio Emission
5%
Excitation
5%
Earth and Planetary Sciences
Emissions
78%
Star Formation
50%
Protostars
32%
Molecular Clouds
23%
Methyl Alcohol
19%
Field Strength
11%
Spectral Energy Distribution
10%
Massive Star
9%
Low Noise
6%
Vapor Phase
6%
Flux Density
6%
Bolometer
5%
Line of Sight
5%
Broadband
5%
Cryogenics
5%
Engineering
Low Noise Amplifier
13%
Monolithic Microwave Integrated Circuits
9%
Gallium Arsenide
7%
Initial Condition
7%
Isothermal
6%
Amplifier
5%