most citedInfrared and X-ray emission of a supernova remnant in a clumpy medium

2 citations · 5 across the 3 of their papers we have counts for

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astro-ph.GA20251 cited

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…

astro-ph.GA20252 cited

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…

astro-ph.GA20252 cited

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…

astro-ph.GA2024

Inhibited destruction of dust by supernova in a clumpy medium

Svyatoslav Yu. Dedikov, Evgenii O. Vasiliev

The decrease rate of dust mass due to strong shock waves ( km s) from supernovae (SNe) estimated for the Milky Way interstellar medium significantly exceeds the…

astro-ph.GA20242 cited

Tracking Dusty Cloud Crushed by a Hot Flow

Svyatoslav Dedikov, Evgenii Vasiliev

The destruction of clouds by strong shocks and hot winds is the key process responsible for the transp orting of metals and dust from the ISM to the ICM/IGM, and establishing the m…