68 citations · 700 across the 45 of their papers we have counts for
48 papers
Computational compressive imaging reconstruction with a simulated-annealing-based Ising solver
Ze Zheng, Xiaoyan Wu, Hang Xu +3
Computational compressive imaging, such as single-pixel imaging and lensless imaging, is a promising imaging technique, enabling the reconstruction of objects from under-sampled me…
High velocity dust grains produced by a supernova explosion
Evgenii O. Vasiliev
Motivated by the discovery of a meteor with velocity more than 300~km/s (Afanasiev et al. 2007) we study how dust grains formed in the supernova (SN) ejecta at its free-expansion p…
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…
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…
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…