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20092026
most citedSupernovae from Red Supergiants with Extensive Mass Loss

163 citations · 894 across the 27 of their papers we have counts for

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astro-ph.SR2022★ 33 cited

Low-luminosity type IIP supernovae: SN 2005cs and SN 2020cxd as very low-energy iron core-collapse explosions

Alexandra Kozyreva, Hans-Thomas Janka, Daniel Kresse +2

SN 2020cxd is a representative of the family of low-energy, underluminous Type IIP supernovae (SNe), whose observations and analysis were recently reported by Yang et al. (2021). H…

astro-ph.SR2021★ 28 cited

Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae

Alexandra Kozyreva, Petr Baklanov, Samuel Jones +2

Stars in the mass range from 8 to 10 solar masses are expected to produce one of two types of supernovae (SNe), either electron-capture supernovae (ECSNe) or core-collapse supernov…

astro-ph.SR2017★ 1 cited

The light curves of type II-P SN 2017eaw: first 200 days

D. Yu. Tsvetkov, S. Yu. Shugarov, I. M. Volkov +7

We present UBVRI photometry of the supernova 2017eaw in NGC 6946, obtained in the period from May 14 until December 7, 2017. We derive dates and magnitudes of maximum light in the…

astro-ph.SR2015★ 1 cited

The Rise-Time of Type II Supernovae

Santiago Gonzalez-Gaitan, N. Tominaga, J. Molina +14

We investigate the early-time light-curves of a large sample of 223 type II supernovae (SNe) from the Sloan Digital Sky Survey and the Supernova Legacy Survey. Having a cadence of…

astro-ph.SR2010★ 163 cited

Supernovae from Red Supergiants with Extensive Mass Loss

Takashi Moriya, Nozomu Tominaga, Sergei I. Blinnikov +2

We calculate multicolor light curves (LCs) of supernovae (SNe) from red supergiants (RSGs) exploded within dense circumstellar medium (CSM). Multicolor LCs are calculated by using…

astro-ph.SR2009★ 5 cited

Photometric observations and modeling of type IIb supernova 2008ax

D. Yu. Tsvetkov, I. M. Volkov, P. V. Baklanov +2

CCD UBVRI photometry is presented for type IIb SN 2008ax for about 320 days. The photometric behavior is typical for core-collapse SNe with low amount of hydrogen. The main photome…