5 papers
Destruction of the interstellar dust by a supernova
Evgenii O. Vasiliev
Destruction of the interstellar dust proceeds primary behind supernova shocks. The previous estimates of the mass of the interstellar dust destroyed in the SN remnant do not take i…
Dust destruction in bubbles driven by multiple supernovae explosions
Evgenii O. Vasiliev, Biman B. Nath
Dust lifetime derived from an isolated supernova (SN) evolution in the interstellar medium is known to be an order of magnitude shorter than the time needed to replenish dust mass…
Interstellar Medium in Extremely High Star-Formation Regions: A Prospect of Observations on the Millimetron Space Observatory
E. O. Vasiliev, S. A. Drozdov, P. V. Baklanov +5
High star-formation rate and active galactic nucleus' emission can significantly transform the interstellar medium. In ultra-luminous infrared galaxies, in which the star-formation…
Far-Infrared Emission from a Late Supernova Remnant in an Inhomogeneous Medium
S. A. Drozdov, S. Yu. Dedikov, E. O. Vasiliev
The interstellar dust grains are swept up during the expansion of the supernova (SN) remnant, they penetrate behind the shock front, where they are heated and destroyed in the hot…
Infrared and X-ray emission of a supernova remnant in a clumpy medium
S. Yu. Dedikov, E. O. Vasiliev
The infrared (IR) to X-ray luminosity ratio (IRX) is an indicator of the role of the dust plays in cooling of hot gas in supernova remnants (SNR). Using the 3D dynamics of gas and…