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Physical Processes of Interstellar Turbulence
Physical Processes Interstellar Turbulence self-gravity radiative heating
2012/2/23
I discuss the role of self-gravity and radiative heating and cooling in shaping the nature of the turbulence in the interstellar medium (ISM) of our galaxy. The heating and cooling cause it to be high...
The observed late-time acceleration of the cosmic expansion constitutes a fundamental problem in modern theoretical physics and cosmology. In an attempt to weight the validity of a large number of dar...
Hii regions in ngc 5055. ii. physical properties。
Physical Interpretation Of Asymmetry Parameter in Galaxies
Effects of the stellar component on derived physical parameters of galactic H II regions
stellar component galactic H II regions physical parameters
2009/6/5
Effects of the stellar component on derived physical parameters of galactic H II regions。
SOME THREE-PARAMETER RELATIONS FOR PHYSICAL CHARACTERISTICS OF STARS
PHYSICAL CHARACTERISTICS STARS
2009/4/8
For homologous stars with μ(ρ, T ) the L-M-Te relation is derived
and tested against an observational material for the main-sequence stars. The transformations
comprising the radius and the surface ...