Bolometric light curves and explosion parameters of 38 stripped-envelope core-collapse supernovae
J. D. Lyman,J. D. Lyman,D. Bersier,Phil A. James,Paolo A. Mazzali,John J. Eldridge,Morgan Fraser,Elena Pian,Elena Pian +8 more
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TLDR
In this article, the bolometric light curve of 38 stripped-envelope core-collapse supernovae (SE SNe) is recovered and template light curves provided.Abstract:
Literature data are collated for 38 stripped-envelope core-collapse supernovae (SE SNe; i.e. SNe IIb, Ib, Ic and Ic-BL) that have good light curve coverage in more than one optical band. Using bolometric corrections derived in previous work, the bolometric light curve of each SN is recovered and template bolometric light curves provided. Peak light distributions and decay rates are investigated; SNe subtypes are not cleanly distinguished in this parameter space, although some grouping of types does occur and there is a suggestion of a Phillips-like relation for most SNe Ic-BL. The bolometric light curves are modelled with a simple analytical prescription and compared to results from more detailed modelling. Distributions of the explosion parameters shows the extreme nature of SNe Ic-BL in terms of their 56Ni mass and the kinetic energy, however ejected masses are similar to other subtypes. SNe Ib and Ic have very similar distributions of explosion parameters, indicating a similarity in progenitors. SNe~IIb are the most homogeneous subtype and have the lowest average values for 56Ni mass, ejected mass, and kinetic energy. Ejecta masses for each subtype and SE SNe as a whole are inconsistent with those expected from very massive stars. The majority of the ejecta mass distribution is well described by more moderately massive progenitors in binaries, indicating these are the dominant progenitor channel for SE SNe.read more
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The Zwicky Transient Facility: Science Objectives
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References
More filters
Journal ArticleDOI
The metamorphosis of SN1998bw
Ferdinando Patat,Enrico Cappellaro,John Danziger,Paolo A. Mazzali,Jesper Sollerman,T. Augusteijn,J. Brewer,V. Doublier,Jean Francois Gonzalez,Olivier Hainaut,Chris Lidman,Bruno Leibundgut,Ken'ichi Nomoto,Takayoshi Nakamura,Jason Spyromilio,Luca Rizzi,Massimo Turatto,Jeremy R. Walsh,Titus Galama,Jan van Paradijs,Chryssa Kouveliotou,Paul Vreeswijk,Filippo Frontera,N. Masetti,Eliana Palazzi,Elena Pian +25 more
TL;DR: In this article, the photometric and spectroscopic evolution of the peculiar SN1998bw, associated with GRB980425, through an analysis of optical and near IR data collected at ESO-La Silla was discussed.
Journal ArticleDOI
Spectropolarimetry of Supernovae
Lifan Wang,J. Craig Wheeler +1 more
TL;DR: In this paper, the authors review the evidence derived from spectropolarimetry that has established several key results: Virtually all supernovae are significantly aspherical near maximum light, core-collapse supernova behave differently than thermonuclear (Type Ia) supernova, and the asphericity of core collapse supernova is more pronounced in the inner layers.
Journal ArticleDOI
No supernovae from two nearby long gamma ray bursts
Johan P. U. Fynbo,Darach Watson,C. C. Thoene,Jesper Sollerman,Joshua S. Bloom,Tamara M. Davis,Jens Hjorth,Pall Jakobsson,U. G. Joergensen,John F. Graham,Andrew S. Fruchter,D. Bersier,Lisa J. Kewley,Arnaud Cassan,José María Castro Cerón,Suzanne Foley,Javier Gorosabel,Tobias C. Hinse,Keith Horne,B. L. Jensen,Sylvio Klose,Daniel Kocevski,J. B. Marquette,Daniel A. Perley,Enrico Ramirez-Ruiz,Maximilian Stritzinger,Paul Vreeswijk,Ralph A. M. J. Wijers,K. Woller,Dong Xu,M. Zub +30 more
TL;DR: In this article, the authors present observations of two nearby long-duration gamma-ray bursts (GRBs) that challenge this simple view, and demonstrate that no SN emission accompanied these longduration bursts, down to limits hundreds of times fainter than the archetypal SN 1998bw that accompanied GRB 980425, and faintter than any Type Ic SN ever observed.
Journal ArticleDOI
A relativistic type Ibc supernova without a detected gamma-ray burst.
Alicia M. Soderberg,Sayan Chakraborti,Giuliano Pignata,Roger A. Chevalier,Poonam Chandra,Alak Ray,M. H. Wieringa,A. Copete,Vandiver Chaplin,Valerie Connaughton,Scott Barthelmy,Michael Bietenholz,N. Chugai,Maximilian Stritzinger,Maximilian Stritzinger,Mario Hamuy,Claes Fransson,Ori Fox,E. M. Levesque,E. M. Levesque,J. E. Grindlay,P. Challis,Ryan J. Foley,Robert P. Kirshner,Peter Milne,Manuel A. P. Torres +25 more
TL;DR: The discovery of luminous radio emission from the seemingly ordinary type Ibc SN 2009bb, which requires a substantial relativistic outflow powered by a central engine, is reported.
Journal ArticleDOI
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TL;DR: A faint type Ib supernova is reported in the halo of the nearby isolated galaxy, NGC 1032, and it is concluded that it arises from a low-mass, old progenitor, likely to have been a helium-accreting white dwarf in a binary.