INIS
gases
100%
protoplanets
98%
mass spectra
95%
clouds
94%
magnetohydrodynamics
93%
magnetic fields
91%
density
77%
fragmentation
75%
stars
70%
size
64%
peaks
60%
angular momentum
47%
dusts
46%
resolution
46%
turbulence
43%
rotation
43%
distribution
42%
feedback
40%
protostars
39%
computerized simulation
39%
hall effect
34%
mass distribution
31%
equations of state
30%
origin
29%
ambipolar diffusion
29%
nonlinear problems
28%
filaments
28%
magnetization
27%
levels
26%
thermodynamics
26%
dynamics
25%
fluctuations
25%
milky way
25%
surveys
25%
h2 regions
23%
simulation
23%
comparative evaluations
21%
emission
21%
friction
21%
luminosity
21%
multiplicity
21%
jets
21%
hydrostatics
21%
ions
21%
maps
21%
red giant stars
21%
instability
21%
compacts
17%
algorithms
16%
universe
14%
Physics
Fragmentation
68%
Stellar Mass
65%
Mass Spectra
43%
Cores
36%
Model
35%
Magnetic Fields
35%
Clouds
31%
Molecular Clouds
30%
Gaseous State
28%
Stars
25%
Magnetohydrodynamics
25%
Magnetization
24%
Simulation
23%
Surveys
21%
Open Cluster
21%
Emission
21%
Protoplanetary Disks
21%
Ion
21%
Plane
21%
Temperature Distribution
21%
Photoelectric Emission
21%
Milky Way
21%
Mass Distribution
21%
High-Mass Stars
21%
Parameter
21%
Regimes
21%
Red Giant Stars
21%
Protoclusters
21%
Friction
21%
Protoplanetary Disk
21%
Magnetohydrodynamics
21%
Diffusivity
21%
Protostars
21%
Gas Cooling
21%
Initial Mass Function
19%
Exponents
17%
Turbulence
15%
Circumstellar Disks
14%
Dust
14%
Algorithms
14%
Ambipolar Diffusion
14%
Behavior
13%
Parsec
10%
Jeans Mass
10%
Equations of State
10%
Hydrostatics
10%
Rotation
10%
Independent Variables
10%
Angular Momentum
10%
Ambipolar Diffusion
10%
Earth and Planetary Sciences
Stellar Mass
43%
Core
27%
Clump
27%
Algorithms
23%
Star Formation
23%
Plane
21%
Dust
21%
Emissions
21%
Comparison
21%
Mass Distribution
21%
Map
21%
Molecular Clouds
21%
Gas
17%
Equation of State
17%
Turbulence
16%
Data Set
16%
Segmentation
16%
Bias
12%
Probability Distribution Function
8%
Condition
7%
Liquid Surface
7%
Counting
7%
Stellar Spectra
7%
Radiative Transfer
7%
Numerical Modeling
7%
Simulation
7%
Sensitivity
7%
Decomposition
5%
Misalignment
5%
Ambipolar Diffusion
5%
Magnetohydrodynamics
5%
Need
5%
Definition
5%
Line of Sight
5%
Standard
5%
High Resolution
5%
Protoplanets
5%
Sample
5%