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相关论文: The Red Supergiant Progenitor of the Type II Super…

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We present a detailed analysis of the progenitor and its local environment for the recently discovered type II supernova (SN) 2024ggi at a distance of about 6.7~Mpc, by utilizing the pre-explosion images from the Hubble Space Telescope…

高能天体物理现象 · 物理学 2024-05-14 Danfeng Xiang , Jun Mo , Xiaofeng Wang , Lingzhi Wang , Jujia Zhang , Han Lin , Liyang Chen , Cuiying Song , Liang-Duan Liu , Zhenyu Wang , Gaici Li

Core-collapse supernovae (SNe) are the spectacular finale to massive stellar evolution. In this Letter, we identify a progenitor for the nearby core-collapse SN 2012aw in both ground based near-infrared, and space based optical…

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 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…

Stellar evolution theory predicts multiple pathways to the explosive deaths of stars as supernovae. Locating and characterizing the progenitors of well-studied supernovae is important to constrain the theory, and to justify and design…

太阳与恒星天体物理 · 物理学 2023-06-21 Joanne L. Pledger , Michael M. Shara

We present early-time photometric and spectroscopic observations of supernova (SN) 2009kr in NGC 1832. We find that its properties to date support its classification as Type II-linear (SN II-L), a relatively rare subclass of core-collapse…

The progenitors of low-luminosity Type II-Plateau supernovae (SNe II-P) are believed to be red supergiant (RSG) stars, but there is much disparity in the literature concerning their mass at core collapse and therefore on the main sequence.…

高能天体物理现象 · 物理学 2017-12-06 Sergey M. Lisakov , Luc Dessart , D. John Hillier , Roni Waldman , Eli Livne

Direct identification of the progenitors of supernovae (SNe) is rare because of the required spatial resolution and depth of the archival data prior to the SN explosions. Here we report on the identification of the progenitors of two nearby…

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,…

天体物理学 · 物理学 2009-11-07 Schuyler D. Van Dyk , Weidong Li , Alexei V. Filippenko

The progenitors of Type II-P supernovae (SN) have been confirmed to be red supergiants. However, the upper mass limit of the directly probed progenitors is much lower than that predicted by current theories, and the accurate determination…

太阳与恒星天体物理 · 物理学 2024-12-03 Xinyi Hong , Ning-Chen Sun , Zexi Niu , Junjie Wu , Qiang Xi , Jifeng Liu

As one of the closest supernovae (SNe) in the last decade, SN 2023ixf is an unprecedented target to investigate the progenitor star that exploded. However, there is still significant uncertainty in the reported progenitor properties. In…

太阳与恒星天体物理 · 物理学 2023-08-31 Ze-Xi Niu , Ning-Chen Sun , Justyn R. Maund , Yu Zhang , Rui-Ning Zhao , Ji-Feng Liu

We present the detection of the progenitor of the Type II SN 2011dh in archival pre-explosion Hubble Space Telescope images. Using post-explosion Adaptive Optics imaging with Gemini NIRI+ALTAIR, the position of the SN in the pre-explosion…

We present the discovery of a red supergiant star that exploded as supernova 2003gd in the nearby spiral galaxy M74. The Hubble Space Telescope (HST) and the Gemini Telescope imaged this galaxy 6 to 9 months before the supernova explosion…

天体物理学 · 物理学 2009-11-10 S. J. Smartt , J. R. Maund , M. A. Hendry , C. A. Tout , G. F. Gilmore , S. Mattila , C. R. Benn

The inevitable fate of massive stars in the initial mass range of ~8--30 M_{Sun} in the red supergiant (RSG) phase is a core-collapse supernova (SN) explosion, although some stars may collapse directly to a black hole. We know that this is…

太阳与恒星天体物理 · 物理学 2025-07-23 Schuyler D. Van Dyk

Supernova (SN) 2024ggi is a nearby Type II SN discovered by ATLAS, showing early flash-ionization features. The pre-explosion images reveal a red supergiant (RSG) progenitor with an initial mass of 10-17 M$_\odot$. In the present work, we…

高能天体物理现象 · 物理学 2025-11-10 Amar Aryan , Erin Higgins , Matt Nicholl , Ting-Wan Chen , Yu-Hsuan Liu

Red supergiants have been confirmed as the progenitor stars of the majority of hydrogen-rich type II supernovae. However, while such stars are observed with masses >25M$_\odot$, detections of >18M$_\odot$ progenitors remain elusive. Red…

Type IIb supernovae are important subclass of stripped-envelope supernovae (SNe), which show H lines only at early times. Their progenitors are believed to contain a low-mass H envelope before explosion. This work reports the discovery of a…

高能天体物理现象 · 物理学 2024-07-08 Zexi Niu , Ning-Chen Sun , Jifeng Liu

Supernova (SN) 2004et is the eighth historical SN in the nearby spiral galaxy NGC 6946. Here we report on early photometric and spectroscopic monitoring of this object. SN 2004et is a Type II event, exhibiting a plateau in its light curves,…

天体物理学 · 物理学 2009-11-10 Weidong Li , Schuyler D. Van Dyk , Alexei V. Filippenko , Jean-Charles Cuillandre

The progenitors of Type II-P supernovae (SNe) are generally considered to be red supergiants; however, the so-called "red supergiant problem" indicates that a deeper investigation into the progenitors of this class of SNe is necessary. SN…

太阳与恒星天体物理 · 物理学 2025-08-04 Yi-Han Zhao , Xinyi Hong , Ning-Chen Sun , Zexi Niu , Justyn R. Maund , Jifeng Liu

Hubble Space Telescope (HST) WFPC2 archival images obtained years prior to the explosion of the Type II-plateau supernova (SN) 2001du in NGC 1365 previously have been analyzed to isolate the progenitor star. The SN site was located using…

天体物理学 · 物理学 2009-11-07 Schuyler D. Van Dyk , Weidong Li , Alexei V. Filippenko
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