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Related papers: The Blue Supergiant Progenitor of the Supernova Im…

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We conducted a search for luminous outbursts prior to the explosion of Type IIn Supernovae (SNe IIn). We built a sample of 27 objects spectroscopically classified as SNe IIn, all located at $z<0.015$. Using deep archival SN fields images…

High Energy Astrophysical Phenomena · Physics 2024-06-19 A. Reguitti , G. Pignata , A. Pastorello , R. Dastidar , D. E. Reichart , J. B. Haislip , V. V. Kouprianov

We report the discovery of a progenitor candidate for the Type~IIb SN2024abfo using multi-epoch pre-explosion images from the Hubble Space Telescope and the Dark Energy Camera Legacy Survey. The progenitor exhibited a ~0.7 mag decline in…

High Energy Astrophysical Phenomena · Physics 2025-06-24 Zexi Niu , Ning-Chen Sun , Justyn R. Maund , Zhen Guo , Wenxiong Li , Meng Sun , Jifeng Liu

The stars that end their lives as supernovae (SNe) have been directly observed in only a handful of cases, due mainly to the extreme difficulty in identifying them in images obtained prior to the SN explosions. Here we report the…

We present HST/WFPC2, GALEX and Chandra observations of the position of the type Ia supernova SN2007sr in the Antennae galaxies, taken before the explosion. No source is found in any of the observations, allowing us to put interesting…

Astrophysics · Physics 2009-11-13 Gijs Nelemans , Rasmus Voss , Gijs Roelofs , Cees Bassa

We obtained late-time optical and near-IR imaging of SN 2008S with the Large Binocular Telescope (LBT), near-IR data with the Hubble Space Telescope (HST), and mid-IR data with the Spitzer Space Telescope (SST). We find that (1) it is again…

Solar and Stellar Astrophysics · Physics 2015-06-04 D. M. Szczygiel , J. L. Prieto , C. S. Kochanek , K. Z. Stanek , T. A. Thompson , J. F. Beacom , P. M. Garnavich , C. E. Woodward

We report evidence for excess blue light from the Type Ia supernova SN 2012cg at fifteen and sixteen days before maximum B-band brightness. The emission is consistent with predictions for the impact of the supernova on a non-degenerate…

We present the results of a detailed, systematic stellar evolution study of binary mergers for blue supergiant (BSG) progenitors of Type II supernovae. In particular, these are the first evolutionary models that can simultaneously reproduce…

Solar and Stellar Astrophysics · Physics 2017-09-11 Athira Menon , Alexander Heger

We present a monitoring study of SN 2004A and probable discovery of a progenitor star in pre-explosion HST images. The photometric and spectroscopic monitoring of SN 2004A show that it was a normal Type II-P which was discovered in NGC 6207…

We consider black hole formation in failed supernovae when a dense circumstellar medium (CSM) is present around the massive star progenitor. By utilizing radiation hydrodynamical simulations, we calculate the mass ejection of blue…

High Energy Astrophysical Phenomena · Physics 2020-07-22 Daichi Tsuna , Ayako Ishii , Naoto Kuriyama , Kazumi Kashiyama , Toshikazu Shigeyama

We present medium-resolution spectroscopy and multicolor photometry for the optical transient PSN J09093496+3307204 (SN 2015bh) in the galaxy NGC 2770, which has transferred into the supernova phase. The observations were carried out…

Solar and Stellar Astrophysics · Physics 2016-09-06 V. P. Goranskij , E. A. Barsukova , A. F. Valeev , D. Yu. Tsvetkov , I. M. Volkov , V. G. Metlov , A. V. Zharova

Identifying the massive progenitor stars that give rise to core-collapse supernovae (SNe) is one of the main pursuits of supernova and stellar evolution studies. Using ground-based images of recent, nearby SNe obtained primarily with KAIT,…

Astrophysics · Physics 2009-11-07 Schuyler D. Van Dyk , Weidong Li , Alexei V. Filippenko

Supernova (SN) iPTF13bvn in NGC 5806 was the first Type Ib SN to have been tentatively associated with a progenitor candidate in pre-explosion images. We performed deep ultraviolet (UV) and optical Hubble Space Telescope (HST) observations…

We present optical and near-infrared (NIR) spectroscopic observations of the nearby Type II supernova SN\,2024ggi from 250 and 581 days after the explosion. Comparing the evolution of the [\ion{O}{1}] at 6300, 6363 \text{\AA} doublet…

We presented a detailed analysis of progenitor properties of type IIP supernova 2017eaw in NGC 6946, based on the pre-explosion images and early-time observations obtained immediately after the explosion. An unusually red star, with…

High Energy Astrophysical Phenomena · Physics 2019-02-27 Liming Rui , Xiaofeng Wang , Jun Mo , Danfeng Xiang , Jujia Zhang , Justyn R. Maund , Avishy Gal-Yam , Lifan Wang , Tianmeng Zhang

We report photometric and spectroscopic observations of the optical transient LSQ13zm. Historical data reveal the presence of an eruptive episode (that we label as `2013a') followed by a much brighter outburst (`2013b') three weeks later,…

Through comparison of pre- and post-explosion images obtained with the Wide Field and Planetary Camera 2 onboard the Hubble Space Telescope, we have isolated a supergiant star prior to explosion at nearly the same position as the…

Solar and Stellar Astrophysics · Physics 2014-11-20 N. Elias-Rosa , S. D. Van Dyk , W. Li , N. Morrell , S. Gonzalez , M. Hamuy , A. V. Filippenko , J. -C. Cuillandre , R. J. Foley , N. Smith

SN Hun248 was classified as a nonterminal eruption (a SN "impostor") from a directly identified and highly variable cool hypergiant star. The 2014 outburst achieved peak luminosity equivalent to that of the historic eruption of luminous…

Solar and Stellar Astrophysics · Physics 2017-12-06 Jon C. Mauerhan , Schuyler D. Van Dyk , Joel Johansson , Ori D. Fox , Alexei V. Filippenko , Melissa L. Graham
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