INIS
protoplanets
100%
gases
92%
magnetohydrodynamics
91%
fragmentation
80%
magnetic fields
78%
mass spectra
78%
clouds
77%
dusts
70%
density
69%
stars
61%
angular momentum
57%
size
56%
protostars
51%
peaks
50%
computerized simulation
47%
distribution
44%
resolution
42%
nonlinear problems
41%
simulation
39%
turbulence
36%
rotation
35%
feedback
33%
equations of state
29%
hall effect
28%
mass distribution
26%
origin
24%
ambipolar diffusion
24%
dynamics
23%
filaments
23%
magnetization
22%
levels
21%
thermodynamics
21%
equations
21%
fluctuations
20%
milky way
20%
surveys
20%
h2 regions
19%
comparative evaluations
18%
emission
18%
friction
18%
luminosity
18%
multiplicity
18%
jets
18%
hydrostatics
18%
ions
18%
maps
18%
red giant stars
18%
instability
18%
constraints
18%
planets
17%
Physics
Fragmentation
56%
Stellar Mass
54%
Mass Spectra
36%
Protostars
36%
Cores
30%
Model
29%
Magnetic Fields
29%
Magnetohydrodynamics
29%
Hydrodynamics
29%
Angular Momentum
27%
Clouds
26%
Molecular Clouds
25%
Gaseous State
23%
Stars
21%
Magnetohydrodynamics
20%
Magnetization
20%
Simulation
19%
Surveys
18%
Open Cluster
18%
Emission
18%
Protoplanetary Disks
18%
Ion
18%
Plane
18%
Temperature Distribution
18%
Photoelectric Emission
18%
Milky Way
18%
Mass Distribution
18%
High-Mass Stars
18%
Parameter
18%
Regimes
18%
Red Giant Stars
18%
Protoclusters
18%
Friction
18%
Protoplanetary Disk
18%
Diffusivity
18%
Gas Cooling
18%
Molecular Clouds
18%
Galerkin Method
18%
Mass Transport
18%
Initial Mass Function
15%
Exponents
14%
Turbulence
12%
Circumstellar Disks
12%
Dust
12%
Algorithms
12%
Ambipolar Diffusion
11%
Behavior
11%
Parsec
9%
Jeans Mass
9%
Equations of State
9%
Earth and Planetary Sciences
Stellar Mass
36%
Core
22%
Clump
22%
Algorithms
19%
Star Formation
19%
Plane
18%
Dust
18%
Emissions
18%
Comparison
18%
Mass Distribution
18%
Map
18%
Molecular Clouds
18%
Gas
14%
Equation of State
14%
Turbulence
13%
Data Set
13%
Segmentation
13%
Bias
10%
Probability Distribution Function
7%
Condition
6%
Liquid Surface
6%
Counting
6%
Stellar Spectra
6%
Radiative Transfer
6%
Numerical Modeling
6%
Simulation
6%
Dichotomy
6%
Equations of State
6%
Sensitivity
5%