1 citations · 5 across the 9 of their papers we have counts for
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Light Curve Models of Supernovae and X-ray spectra of Supernova Remnants
S. I. Blinnikov, P. V. Baklanov, A. V. Kozyreva +1
We compare parameters of well-observed type II SN1999em derived by M.Hamuy and D.Nadyozhin based on Litvinova-Nadyozhin (1985) analytic fits with those found from the simulations w…
SN 1994W: evidence of explosive mass ejection a few years before explosion
Nikolai N. Chugai, Robert J. Cumming, Sergei I. Blinnikov +7
We present and analyse spectra of the Type IIn supernova 1994W obtained between 18 and 202 days after explosion. During the first 100 days the line profiles are composed of three m…
Lightcurves of thermonuclear supernovae as a probe of the explosion mechanism and their use in cosmology
S. Blinnikov, E. Sorokina
Thermonuclear supernovae are valuable for cosmology but their physics is not yet fully understood. Modeling the development and propagation of nuclear flame is complicated by numer…
Shock breakouts in SNe Ib/c
S. I. Blinnikov, D. K. Nadyozhin, S. E. Woosley +1
Numerical modeling of shock breakout in compact presupernovae of type Ib/c is done by two independent methods. Peak color temperatures reach 4 to 8 million K for explosion energies…
X-ray emission of young SN Ia remnants as a probe for an explosion model
D. I. Kosenko, E. I. Sorokina, S. I. Blinnikov +1
We present results of hydrodynamical simulations of young supernova remnants. To model the ejecta, we use several models (discussed in literature) of type Ia supernova explosions w…
Energy exchange inside SN ejecta and light curves of SNe Ia
E. I. Sorokina, S. I. Blinnikov
A treatment of line opacity in expanding medium is most crucial for the light curve (LC) modeling of Type Ia supernovae (SNe Ia). Spectral lines are the main source of opacity insi…