Physics & Astronomy
star formation
100%
gases
65%
star formation rate
62%
molecular clouds
62%
stars
56%
galaxies
53%
simulation
46%
turbulence
39%
molecular gases
36%
supernovae
32%
disk galaxies
25%
hydrodynamics
24%
spiral galaxies
22%
kinematics
20%
shock
18%
cosmic rays
17%
gravitation
17%
magnetic fields
17%
momentum
16%
thermal instability
15%
cooling
15%
magnetohydrodynamic simulation
15%
radiation
14%
magnetohydrodynamics
14%
star clusters
13%
massive stars
12%
galactic winds
12%
solar neighborhood
11%
dust
11%
filaments
11%
chemistry
10%
metallicity
10%
clumps
10%
astrophysics
10%
accretion disks
9%
heating
9%
stellar winds
9%
shearing
9%
free fall
9%
estimates
9%
gravitational fields
8%
radii
8%
field strength
8%
depletion
7%
angular momentum
7%
tracers
7%
magnetohydrodynamic turbulence
7%
radiation pressure
7%
luminosity
7%
turbulent mixing
7%
ambipolar diffusion
7%
ionized gases
7%
bows
7%
high resolution
6%
velocity distribution
6%
bubbles
6%
gradients
6%
escape
6%
energy
6%
ionization
6%
temperature
6%
high temperature gases
6%
fractals
6%
coalescing
6%
optical thickness
6%
shear
6%
profiles
5%
monatomic gases
5%
expansion
5%
sheaths
5%
dissipation
5%
scale height
5%
cylindrical coordinates
5%
injection
5%
substructures
5%
Earth & Environmental Sciences
gas
92%
simulation
59%
turbulence
45%
magnetohydrodynamics
42%
outflow
42%
magnetic field
36%
rate
29%
hydrodynamics
26%
momentum
25%
accretion
25%
radiation
22%
cosmic ray
22%
angular momentum
20%
kinematics
18%
gravity
18%
cooling
17%
young
15%
cold
15%
energy
14%
regulation
14%
heating
12%
shell
12%
luminosity
11%
dust
10%
ionization
10%
temperature
9%
feather
9%
parameter
9%
speed
8%
code
8%
modeling
7%
bubble
7%
fountain
7%
inflow
7%
merger
7%
coalescence
6%
optical depth
6%
loss
6%
turbulent mixing
6%
distribution
6%
power law
6%
particle
6%
dissipation
6%
hydrogen
6%
energetics
5%
ray tracing
5%
explosion
5%
ion
5%
tracer
5%
test
5%
physics
5%
transition
5%
perturbation
5%
Coriolis force
5%
geometry
5%
torque
5%
astronomy
5%
