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We investigate the fundamental properties of core-collapse Supernova (SN) progenitors from single stars at solar metallicity. We combine Geneva stellar evolutionary models with initial masses of Mini=20-120 Msun with atmospheric/wind models…

Solar and Stellar Astrophysics · Physics 2015-06-17 Jose H. Groh , Georges Meynet , Cyril Georgy , Sylvia Ekstrom

As most massive stars are born in binary and other multiple-star systems, many are expected to exchange mass with a companion star or merge with it during their lives. This means that most supernovae (SNe) are from such binary products.…

High Energy Astrophysical Phenomena · Physics 2025-08-27 F. R. N. Schneider , E. Laplace , Ph. Podsiadlowski

We have developed a detailed stellar evolution code capable of following the simultaneous evolution of both stars in a binary system, together with their orbital properties. To demonstrate the capabilities of the code we investigate…

Solar and Stellar Astrophysics · Physics 2015-05-13 Richard J. Stancliffe , John J. Eldridge

Red supergiants (RSGs), which are progenitors of hydrogen-rich Type II supernovae (SNe), have been known to pulsate from both observations and theory. The pulsations can be present at core collapse and affect the resulting SN. However, SN…

Solar and Stellar Astrophysics · Physics 2025-11-12 V. A. Bronner , E. Laplace , F. R. N. Schneider , Ph. Podsiadlowski

We present observations of SN2009hd in the nearby galaxy M66. This SN is one of the closest to us in recent years but heavily obscured by dust, rendering it unusually faint in the optical, given its proximity. We find that the observed…

The current perspective about the explosions of massive hydrogen-rich blue supergiants is that they resemble SN 1987A. These so-called peculiar Type II supernovae, however, are one of the rarest types of supernovae and may not hence be the…

High Energy Astrophysical Phenomena · Physics 2025-01-17 Takashi J. Moriya , Athira Menon

Observations spanning a large wavelength range, from X-ray to radio, of the Type IIb supernova 2011hs are presented, covering its evolution during the first year after explosion. The optical light curve presents a narrower shape and a…

Evolutionary effects with redshift of core collapse supernovae and their application to cosmology have been studied based on an extensive grid of stellar models between 13 and 25 Mo, and their light curves after the explosion. With…

Astrophysics · Physics 2007-05-23 P. Höflich , O. Straniero , M. Limongi , I. Dominguez , A. Chieffi

(Abridged) We present a search for the progenitor star of the Type Ic Supernova 2002ap in deep, high quality pre-explosion observations taken with the Canada-France-Hawaii Telescope (CFHT). Aligning high-resolution Hubble Space Telescope…

Type IIb Supernova (SN) 2011dh, with conclusive detection of an unprecedented Yellow Supergiant (YSG) progenitor, provides an excellent opportunity to deepen our understanding on the massive star evolution in the final centuries toward the…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Keiichi Maeda , Satoru Katsuda , Aya Bamba , Yukikatsu Terada , Yasushi Fukazawa

We present Hubble Space Telescope (HST) observations of the type IIb supernova (SN) 2016gkg at 652, 1698, and 1795 days with the Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). Comparing to pre-explosion imaging from 2001…

High Energy Astrophysical Phenomena · Physics 2022-09-14 Charles D. Kilpatrick , David A. Coulter , Ryan J. Foley , Anthony L. Piro , Armin Rest , César Rojas-Bravo , Matthew R. Siebert

We present a detection in pre-explosion Hubble Space Telescope (HST) imaging of a point source consistent with being the progenitor star of the Type IIb supernova (SN IIb) 2016gkg. Post-explosion imaging from the Keck Adaptive Optics system…

The availability of updated model atmospheres for red supergiants and improvements in single and binary stellar evolution models, as well as previously unpublished data prompted us to revisit the progenitor of low-luminosity type II-Plateau…

Solar and Stellar Astrophysics · Physics 2021-01-13 D. O'Neill , R. Kotak , M. Fraser , S. Mattila , G. Pietrzyński , J. L. Prieto

Little is observationally known about the progenitors of Type Ibc supernovae (SNe) or the typical activity of SNe progenitors in their final years. Here, we analyze deep Large Binocular Telescope imaging data spanning the 4 years before and…

Solar and Stellar Astrophysics · Physics 2017-10-18 Samson A. Johnson , C. S. Kochanek , S. M. Adams

We present optical and near-infrared observations of the rapidly evolving supernova (SN) 2017czd that shows hydrogen features. The optical light curves exhibit a short plateau phase ($\sim 13$ days in the $R$-band) followed by a rapid…

Since the discovery of SN (supernova) 1987A, the number of Type II-peculiar SNe has grown, revealing a rich diversity in photometric and spectroscopic properties. In this study, using a single 15Msun low-metallicity progenitor that dies as…

Solar and Stellar Astrophysics · Physics 2018-12-20 Luc Dessart , D. John Hillier

Linking supernovae to their progenitors is a powerful method for furthering our understanding of the physical origin of their observed differences, while at the same time testing stellar evolution theory. In this second study of a series of…

The progenitors of many type II core-collapse supernovae have now been identified directly on pre-discovery imaging. Here we present an extensive search for the progenitors of type Ibc supernovae in all available pre-discovery imaging since…

Solar and Stellar Astrophysics · Physics 2015-06-12 John J. Eldridge , Morgan Fraser , Stephen J. Smartt , Justyn R. Maund , R. Mark Crockett

We have obtained limited photometric and spectroscopic data for Supernova (SN) 2008bk in NGC 7793, primarily at >~ 150 d after explosion. We find that it is a Type II-Plateau (II-P) SN which most closely resembles the low-luminosity SN…

From stellar evolution simulations (using MESA) we conclude that the fatal common envelope evolution (CEE) channel for the formation of Type IIb core collapse supernova (SN IIb) progenitors can indeed account for some SNe IIb. In the fatal…

High Energy Astrophysical Phenomena · Physics 2019-09-25 Noam Lohev , Efrat Sabach , Avishai Gilkis , Noam Soker
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