scholarly journals Numerical Simulation of the Thermal Turbulence in the Optical Thick Clouds of the Interstellar Medium

Author(s):  
Vitaliy Korolev ◽  
Mikhail Eremin ◽  
Elena Zhukova ◽  
Ilya Kovalenko ◽  
Andrey Zankovich
2012 ◽  
Vol 8 (S291) ◽  
pp. 527-529
Author(s):  
O. M. Ulyanov ◽  
A. A. Seredkina ◽  
A. I. Shevtsova

AbstractWe give a new numerical model of pulsar pulse radiation through the interstellar medium (ISM) considering the propagation effects. It explains the deficit of a scattering measure at the decameter range of frequencies that leads to the possibility of detecting the pulsar pulse fine structure. The results of numerical simulation confirm that the fine structure may be detected at low frequencies and this is qualitatively agreed with the observational data.


1999 ◽  
Vol 186 ◽  
pp. 213-216
Author(s):  
Jeroen P.E. Gerritsen ◽  
Vincent Icke

We present a numerical simulation of two merging equal-mass, gas-rich disk galaxies. Special emphasis is given to an accurate treatment of the interstellar medium physics and star formation with its feedback. We will explain how the negative feedback from young stars restricts the bulk of the star formation during the merger-induced starburst to the nucleus.


2005 ◽  
Vol 358 (3) ◽  
pp. 705-715 ◽  
Author(s):  
S. V. Bogovalov ◽  
V. M. Chechetkin ◽  
A. V. Koldoba ◽  
G. V. Ustyugova

2009 ◽  
Vol 00 (00) ◽  
pp. 090904073309027-8
Author(s):  
H.W. Wang ◽  
S. Kyriacos ◽  
L. Cartilier

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