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Related papers: Type Ib/c Supernovae with and without Gamma-Ray Bu…

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We investigate the influence of close neighbor galaxies on the properties of supernovae (SNe) and their host galaxies using 56 SNe located in pairs of galaxies with different levels of star formation (SF) and nuclear activity. The mean…

Cosmology and Nongalactic Astrophysics · Physics 2014-08-26 T. A. Nazaryan , A. R. Petrosian , A. A. Hakobyan , V. Zh. Adibekyan , D. Kunth , G. A. Mamon , M. Turatto , L. S. Aramyan

The properties of supernovae (SNe) are reviewed. It is shown that the observed characteristics of the morphological classes of SNe (types Ia, Ib/c, II) can be explained in terms of two basic explosion mechanisms, i.e. core collapse of…

Astrophysics · Physics 2017-08-23 Nino Panagia

Context. Some circumstellar-interacting (CSI) supernovae (SNe) are produced by the explosions of massive stars that have lost mass shortly before the SN explosion. There is evidence that the precursors of some SNe IIn were luminous blue…

High Energy Astrophysical Phenomena · Physics 2015-08-19 F. Taddia , J. Sollerman , C. Fremling , A. Pastorello , G. Leloudas , C. Fransson , A. Nyholm , M. D. Stritzinger , M. Ergon , R. Roy , K. Migotto

Broad-lined type Ic supernovae (SNe Ic-BL) are peculiar stellar explosions that distinguish themselves from ordinary SNe. Some SNe Ic-BL are associated with long-duration (\gtrsim 2 s) gamma-ray bursts (GRBs). Black holes and magnetars are…

High Energy Astrophysical Phenomena · Physics 2017-03-22 L. J. Wang , H. Yu , L. D. Liu , S. Q. Wang , Y. H. Han , D. Xu , Z. G. Dai , Y. L. Qiu , J. Y. Wei

Type IIb supernovae (SNe IIb) present a unique opportunity for investigating the evolutionary channels and mechanisms governing the evolution of stripped-envelope SN progenitors due to a variety of observational constraints available.…

High Energy Astrophysical Phenomena · Physics 2020-11-11 Niharika Sravan , Pablo Marchant , Vassiliki Kalogera , Dan Milisavljevic , Raffaella Margutti

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-peaked morphology, which is among Type Ib/Ic supernovae. The…

Stripped-envelope supernovae (Types IIb, Ib, and Ic) that show little or no hydrogen comprise roughly one-third of the observed explosions of massive stars. Their origin and the evolution of their progenitors are not yet fully understood.…

Gamma Ray Burst (GRBs) are empirically classified as long-duration GRBs (LGRBs, $>$ 2s) and short-duration GRBs (SGRBs, $<$ 2s). Physically they can be grouped into two distinct progenitor categories: those originating from collapse of…

High Energy Astrophysical Phenomena · Physics 2020-07-22 Ye Li , Bing Zhang , Qiang Yuan

The connection between long GRBs and supernovae is now well established. I briefly review the evidence in favor of this connection and summarise where we are observationally. I also use a few events to exemplify what should be done and what…

High Energy Astrophysical Phenomena · Physics 2012-07-02 David Bersier

I use photometry and spectroscopy data for 24 Type II plateau supernovae to examine their observed and physical properties. This dataset shows that these objects encompass a wide range of ~5 mag in their plateau luminosities, their…

Astrophysics · Physics 2010-04-06 Mario Hamuy

Throughout the last 20 years 7 supernovae (SNe) have been discovered within Arp 299. One of these is unclassified, leaving 6 core-collapse events; 2 type II, 2 type Ib, a type IIb and one object of indistinct type; Ib/IIb. We analyse the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 J. P. Anderson , S. M. Habergham , P. A. James

The duration of a gamma-ray burst (GRB) is a key indicator of its physics origin, with long bursts perhaps associated with the collapse of massive stars and short bursts with mergers of neutron stars.However, there is substantial overlap in…

There are indications that $\gamma$-ray dark objects such as supernovae (SNe) with choked jets, and the cores of active galactic nuclei may contribute to the diffuse flux of astrophysical neutrinos measured by the IceCube observatory. In…

High Energy Astrophysical Phenomena · Physics 2018-01-23 Nicholas Senno , Kohta Murase , Peter Mészáros

The supernovae of Type Ibc are rare and the detailed characteristics of these explosions have been studied only for a few events. Unlike Type II SNe, the progenitors of Type Ibc have never been detected in pre-explosion images. So, to…

Studying the nature of various types of supernovae (SNe) is important for our understanding of stellar evolution. Observations of atomic and molecular gas in the host galaxies of gamma-ray bursts (GRBs) and SNe have recently been used to…

Astrophysics of Galaxies · Physics 2020-07-01 Michał J. Michałowski , Natalia Gotkiewicz , Jens Hjorth , Peter Kamphuis

We present a method designed to identify the spectral type of young (less than ~30 days after explosion) and nearby (z < ~0.05) supernovae (SNe) using their broad-band colors. In particular, we show that stripped-core SNe (i.e., hydrogen…

Astrophysics · Physics 2009-11-10 Avishay Gal-Yam , Dovi Poznanski , Dan Maoz , Alexei V. Filippenko , Ryan J. Foley

The pursuit of the progenitors of short duration-hard spectrum gamma-ray bursts (SHBs) draws strongly upon similar quests for the origin of supernovae (SNe) and long duration-soft spectrum GRBs(LSBs). Indeed the notion that, in the absence…

Astrophysics · Physics 2009-11-11 J. S. Bloom , J. X. Prochaska

This paper reports an environmental analysis of 41 uniformly-selected stripped-envelope supernovae (SESNe) based on deep ultraviolet-optical images acquired by the Hubble Space Telescope. Young stellar populations are detected in most SN…

Solar and Stellar Astrophysics · Physics 2023-03-15 Ning-Chen Sun , Justyn R. Maund , Paul A. Crowther

The discovery of supernovae associated with long-duration gamma ray burst observations is primary evidence that the progenitors of these outbursts are massive stars. One of the principle mysteries in understanding these progenitors has been…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Lucille H. Frey , Chris L. Fryer , Patrick A. Young

Spectroscopic and spectropolarimetric observations of SN 2003dh/GRB 030329 obtained in 2003 May using the Subaru 8.2 m telescope are presented. The properties of the SN are investigated through a comparison with spectra of the Type Ic…