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Related papers: The He-rich core-collapse supernova 2007Y: Observa…

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We present a theoretical model for Type Ib supernova (SN) 2006jc. We calculate the evolution of the progenitor star, hydrodynamics and nucleosynthesis of the SN explosion, and the SN bolometric light curve (LC). The synthetic bolometric LC…

We present 1-D non-Local-Thermodynamic-Equilibrium time-dependent radiative-transfer simulations for supernovae (SNe) of type IIb, Ib, and Ic that result from the terminal explosion of the mass donor in a close-binary system. Here, we…

Solar and Stellar Astrophysics · Physics 2015-09-09 Luc Dessart , D. John Hillier , Stan Woosley , Eli Livne , Roni Waldman , Sung-Chul Yoon , Norbert Langer

The nature of the peculiar `Ca-rich' SN 2019ehk in the nearby galaxy M100 remains unclear. Its origin has been debated as either a stripped core-collapse supernova or a thermonuclear helium detonation event. Here, we present very late-time…

High Energy Astrophysical Phenomena · Physics 2021-01-27 Kishalay De , U. Christoffer Fremling , Avishay Gal-Yam , Ofer Yaron , Mansi M. Kasliwal , S. R. Kulkarni

The optical and ultra-violet broadband photometric and spectroscopic observations of the Type II supernova (SN) 2016gfy are presented. The $V$-band light curve (LC) shows a distinct plateau phase with a slope, $s_2$ $\sim$ 0.12 mag / 100 d…

High Energy Astrophysical Phenomena · Physics 2019-09-11 Avinash Singh , Brajesh Kumar , Takashi J. Moriya , G. C. Anupama , D. K. Sahu , Peter J. Brown , Jennifer E. Andrews , Nathan Smith

We present optical observations of the Type IIb supernova (SN) 2017ckj, covering approximately 180 days after the explosion. Its early-time multi-band light curves display no clear evidence of a shock-cooling tail, resembling the behavior…

Using the Monte Carlo code, SEDONA, multiband photometry and spectra are calculated for supernovae derived from stripped helium stars with presupernova masses from 2.2 to 10.0 $M_\odot$. The models are representative of evolution in close…

High Energy Astrophysical Phenomena · Physics 2021-06-23 Stan Woosley , Tuguldur Sukhbold , Daniel Kasen

We investigate the possibility of a super-luminous Type Ic core-collapse supernovae producing a large amount of 56Ni. Very massive stars with a main-sequence mass larger than 100 Msun and a metallicity 0.001 < Z < 0.004 are expected to…

Solar and Stellar Astrophysics · Physics 2015-06-18 Takashi Yoshida , Shinpei Okita , Hideyuki Umeda

Supernova (SN) 2008bk is a well observed low-luminosity Type II event visually associated with a low-mass red-supergiant progenitor. To model SN 2008bk, we evolve a 12Msun star from the main sequence until core collapse, when it has a total…

Solar and Stellar Astrophysics · Physics 2017-01-18 Sergey Lisakov , Luc Dessart , D. John Hillier , Roni Waldman , Eli Livne

In this paper we present the results of the radio light curve and X-ray observations of broad-lined Type Ic SN 2007bg. The light curve shows three distinct phases of spectral and temporal evolution, implying that the SNe shock likely…

High Energy Astrophysical Phenomena · Physics 2012-10-10 P. Salas , F. E. Bauer , C. Stockdale , J. L. Prieto

We present extensive radio and X-ray observations of SN\, 2012au, the energetic radio luminous supernova of type Ib that may be a link between subsets of hydrogen-poor superluminous and normal core-collapse supernovae. The observations…

Optical $UBVRI$ photometry and medium resolution spectroscopy of the type Ib supernova SN 2009jf, during the period $\sim -15$ to +250days with respect to the $B$ maximum are reported. The light curves are broad, with an extremely slow…

Solar and Stellar Astrophysics · Physics 2015-05-27 D. K. Sahu , U. K. Gurugubelli , G. C. Anupama , K. Nomoto

A set of hydrodynamical models based on stellar evolutionary progenitors is used to study the nature of SN 2011dh. Our modeling suggests that a large progenitor star ---with R ~200 Rsun---, is needed to reproduce the early light curve of SN…

Aim. We present and interpret the data of the nearby hydrogen-deficient but helium-rich superluminous supernova SN~2021bnw which reached a magnitude of -20.7 at maximum luminosity in g band. Methods. We discuss the light curves and spectra…

We present nebular phase optical and near-infrared spectroscopy of the Type Ia supernova (SN) 2017cbv. The early light curves of SN~2017cbv showed a prominent blue bump in the $U$, $B$ and $g$ bands lasting for $\sim$5 d. One interpretation…

SN 2007bi and SN 1999as are among the first superluminous supernovae discovered. SN 2007bi was suggested to be powered by the radioactive decay of a large amount (5 - 10 Msun) of 56Ni. SN 1999as has a similar spectrum to SN 2007bi. One…

High Energy Astrophysical Phenomena · Physics 2019-02-20 Takashi J. Moriya , Paolo A. Mazzali , Masaomi Tanaka

We present optical photometry and spectra for the Type Ia supernova (SN Ia) 2007gi in the nearby galaxy NGC 4036. SN 2007gi is characterized by extremely high-velocity (HV) features of the intermediate-mass elements (Si, Ca, and S), with…

Solar and Stellar Astrophysics · Physics 2015-05-14 T. Zhang , X. Wang , W. Li , A. V. Filippenko , L. Wang , X. Zhou , P. J. Brown , J. M. Silverman , T. N. Steele , M. Ganeshalingam , J. Li , J. Deng , T. Li , Y. Qiu , M. Zhai , R. Shang

SN 2013dy is a Type Ia supernova for which we have compiled an extraordinary dataset spanning from 0.1 to ~ 500 days after explosion. We present 10 epochs of ultraviolet (UV) through near-infrared (NIR) spectra with HST/STIS, 47 epochs of…

We present nonlocal thermodynamic equilibrium radiative transfer calculations of red supergiant and He-star explosions, extending previous work to focus on the infrared emission from atoms and ions in the ejecta during the nebular-phase…

Solar and Stellar Astrophysics · Physics 2026-01-14 Luc Dessart

Supernova (SN) 2017cbv in NGC 5643 is one of a handful of type Ia supernovae (SNe~Ia) reported to have excess blue emission at early times. This paper presents extensive $BVRIYJHK_s$-band light curves of SN 2017cbv, covering the phase from…

We present optical UBVRI photometry and medium resolution spectroscopy of the type Ib supernova iPTF13bvn, spanning a phase of $\sim$ $-13\,$d to $+71\,$d with respect to $B$-band maximum. The post maximum decline rates indicate a fast…

Solar and Stellar Astrophysics · Physics 2015-06-22 Shubham Srivastav , G. C. Anupama , D. K. Sahu