activity
19992008
most citedTheoretical light curves for deflagration models of Type Ia supernova

280 citations · 316 across the 5 of their papers we have counts for

collaborators
Showing astro-phShow all

12 papers · 1 filter

astro-ph200835 cited

XMM-Newton X-ray spectra of the SNR 0509-67.5: data and models

D. Kosenko, J. Vink, S. Blinnikov +1

We report on X-ray observations of the supernova remnant 0509-67.5 in the Large Magellanic Cloud with XMM-Newton X-ray observatory. We use the imaging spectroscopy (EPIC) and Refle…

astro-ph2006280 cited

Theoretical light curves for deflagration models of Type Ia supernova

S. I. Blinnikov, F. K. Roepke, E. I. Sorokina +5

We present synthetic bolometric and broad-band UBVRI light curves of SNe Ia, for four selected 3-D deflagration models of thermonuclear supernovae. The light curves are computed wi…

astro-ph2005

SN 2005bf: A Possible Transition Event Between Type Ib/c Supernovae and Gamma Ray Bursts

Gaston Folatelli, Carlos Contreras, M. M. Phillips +22

We present u'g'r'i'BV photometry and optical spectroscopy of the Type Ib/Ic SN 2005bf covering the first ~100 days following discovery. The u'g'BV light curves displayed a double-p…

astro-ph2005

New Studies of the Pulsar Wind Nebula in the Supernova Remnant CTB 80

T. A. Lozinskaya, V. N. Komarova, A. V. Moiseev +1

We investigated the kinematics of the pulsar wind nebula (PWN) associated with PSR B1951+32 in the old supernova remnant CTB 80 using the Fabry-Perot interferometer of the 6m Speci…

astro-ph2004

Photometric Observations of the Type Ia SN 2002er in UGC 10743

G. Pignata, F. Patat, S. Benetti +20

Extensive light and colour curves for the Type Ia supernova SN 2002er are presented as part of the European Supernova Collaboration. We have collected UBVRI photometry from ten dif…

astro-ph2004

The type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope

Nikolai N. Chugai, Sergei I. Blinnikov, Robert J. Cumming +6

We present and analyse spectra of the Type IIn supernova 1994W obtained between 18 and 203 days after explosion. During the luminous phase (first 100 d) the line profiles are compo…