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Related papers: Oxygen and helium in stripped-envelope supernovae

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Super-luminous supernovae (SLSNe) are tremendously luminous explosions whose power sources and progenitors are highly debated. Broad-lined SNe Ic (SNe Ic-bl) are the only type of SNe that are connected with long-duration gamma ray bursts…

High Energy Astrophysical Phenomena · Physics 2017-08-23 Yu-Qian Liu , Maryam Modjaz , Federica B. Bianco

An analysis leveraging 170 optical spectra of 35 stripped-envelope (SE) core-collapse supernovae observed by the Carnegie Supernova Project-I and published in a companion paper is presented. Mean template spectra are constructed for the SNe…

In Paper I of this series, we showed that the ratio between stripped-envelope (SE) supernova (SN) and Type II SN rates reveals a significant SE SN deficiency in galaxies with stellar masses $\lesssim 10^{10}~{\rm M}_\odot$. Here, we test…

High Energy Astrophysical Phenomena · Physics 2017-03-13 Or Graur , Federica B. Bianco , Maryam Modjaz , Isaac Shivvers , Alexei V. Filippenko , Weidong Li , Nathan Smith

Stripped-envelope supernovae (SE-SNe) show a wide variety of photometric and spectroscopic properties. This is due to the different potential formation channels and the stripping mechanism that allows for a large diversity within the…

The spectroscopic properties of a selected optical photospheric spectra of core collapse supernovae (CCSNe) are investigated.Special attention is devoted to traces of hydrogen at early phases. The generated spectra are found to match the…

Astrophysics · Physics 2009-11-11 A. Elmhamdi , I. J. Danziger , D. Branch , B. Leibundgut , E. Baron , R. P. Kirshner

The optical and optical/near-infrared pseudo-bolometric light curves of 85 stripped-envelope supernovae (SNe) are constructed using a consistent method and a standard cosmology. The light curves are analysed to derive temporal…

The dominant mechanism and time scales over which stripped-envelope supernovae (SNe) progenitor stars shed their hydrogen envelopes are uncertain. Observations of Type Ib and Ic SNe at late phases could reveal the optical signatures of…

Solar and Stellar Astrophysics · Physics 2018-06-13 Jon C. Mauerhan , Alexei V. Filippenko , Weikang Zheng , Thomas Brink , Melissa L. Graham , Isaac Shivvers , Kelsey Clubb

Among the supernovae (SNe) that show strong interaction with the circumstellar medium, there is a rare subclass of Type Ia supernovae, SNe Ia-CSM, that show strong narrow hydrogen emission lines much like SNe IIn but on top of a diluted…

Type Ib and Ic supernovae (SNe Ib/Ic) are the bright finale of massive stars that have lost their hydrogen envelopes, making them powerful probes of mass stripping in massive star evolution. The advent of modern large photometric and…

High Energy Astrophysical Phenomena · Physics 2026-05-05 Harim Jin , Selma E. de Mink , Sebastian Holzner , Jakub Klencki , Géza Csörnyei , Sung-Chul Yoon , Iair Arcavi , Wolfgang E. Kerzendorf

I present an overview of optical observations (mostly spectra) of Type II, Ib, and Ic supernovae (SNe). SNe II are defined by the presence of hydrogen, and exhibit a very wide variety of properties. SNe II-L tend to show evidence of…

Astrophysics · Physics 2009-11-06 Alexei V. Filippenko

We analyse spectroscopic measurements of 122 type Ia supernovae (SNe Ia) with z<0.09 discovered by the Palomar Transient Factory, focusing on the properties of the Si II 6355 and Ca II `near-infrared triplet' absorptions. We examine the…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Y. -C. Pan , M. Sullivan , K. Maguire , A. Gal-Yam , I. M. Hook , D. A. Howell , P. E. Nugent , P. A. Mazzali

We present observations of two new hydrogen-poor superluminous supernovae (SLSN-I), iPTF15esb and iPTF16bad, showing late-time H-alpha emission with line luminosities of (1-3)e+41 erg/s and velocity widths of (4000-6000) km/s. Including the…

We present a comprehensive analysis of the early spectra of type II and type IIb supernovae (SNe) to explore their diversity and distinguishable characteristics. Using 866 publicly available spectra from 393 SNe, 407 from type IIb SNe (SNe…

High Energy Astrophysical Phenomena · Physics 2025-07-14 Maider González-Bañuelos , Claudia P. Gutiérrez , Lluís Galbany , Santiago González-Gaitán

The velocities and equivalent widths (EWs) of a set of absorption features are measured for a sample of 28 well-observed Type Ia supernovae (SN Ia) covering a wide range of properties. The values of these quantities at maximum are obtained…

Astrophysics · Physics 2008-11-26 S. Hachinger , P. A. Mazzali , S. Benetti

We present 75 near-infrared (NIR; 0.8$-$2.5 $\mu$m) spectra of 34 stripped-envelope core-collapse supernovae (SESNe) obtained by the Carnegie Supernova Project-II (CSP-II), encompassing optical spectroscopic Types IIb, Ib, Ic, and Ic-BL.…

Unlike the ordinary supernovae (SNe) some of which are hydrogen and helium deficient (called Type Ic SNe), broad-lined Type Ic SNe (SNe Ic-bl) are very energetic events, and all SNe coincident with bona fide long duration gamma-ray bursts…

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

We present six epochs of spectropolarimetric observations and one epoch of spectroscopy of the Type Ib SN iPTF 13bvn. The epochs of these observations correspond to $-$10 to $+$61 days with respect to the {\it r}-band light curve maximum.…

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…

Solar and Stellar Astrophysics · Physics 2016-02-03 Joe Lyman , David Bersier , Phil James , Paolo Mazzali , John Eldridge , Morgan Fraser , Elena Pian