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相关论文: A Study of the Type II-P Supernova 2003gd in M74

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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

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…

HST WFPC2 archival F606W and F300W images obtained within one year prior to the explosion of the nearby Type II supernova (SN) 2003gd in Messier 74 (NGC 628) have been analyzed to isolate the progenitor star. The SN site was located using…

天体物理学 · 物理学 2009-02-24 S. D. Van Dyk , W. Li , A. V. Filippenko

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

We present extensive ultraviolet, optical, and near-infrared observations of the type IIP supernova (SN IIP) 2013ej in the nearby spiral galaxy M74. The multicolor light curves, spanning from $\sim$ 8--185 days after explosion, show that it…

We present mid-infrared observations with the Spitzer Space Telescope of the nearby type II-P supernova, SN 2004dj, at epochs of 89 to 129 days. We have obtained the first mid-IR spectra of any supernova apart from SN 1987A. A prominent…

天体物理学 · 物理学 2009-11-13 Rubina Kotak , Peter Meikle , Schuyler van Dyk , Peter Hoeflich , Seppo Mattila

We present early photometric and spectroscopic observations of SN 2013ej, a bright type IIP supernova in M74. SN 2013ej is one of the closest SNe ever discovered. The available archive images and the early discovery help to constrain the…

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 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…

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

M74 (NGC 628) is a famous face-on spiral galaxy, hosting three core-collapse supernovae (SNe):SN Ic 2002ap, SN II-P 2003gd, and SN II-P 2013ej. However its distance is not well known. We present a distance estimation for this galaxy based…

星系天体物理 · 物理学 2015-06-22 In Sung Jang , Myung Gyoon Lee

We present high quality ground-based VRI images of the site of the Type II-P SN1999em (in NGC1637) taken before explosion, which were extracted from the CFHT archive. We determine a precise position of the SN on these images to an accuracy…

天体物理学 · 物理学 2009-11-06 S. J. Smartt , G. F. Gilmore , C. A. Tout , S. T. Hodgkin

The pre-explosion observations of the type II-P supernovae 2006my, 2006ov and 2004et, are re-analysed. In the cases of supernovae 2006my and 2006ov we argue that the published candidate progenitors are not coincident with their respective…

宇宙学与河外天体物理 · 物理学 2015-05-14 R. M. Crockett , S. J. Smartt , A. Pastorello , J. J. Eldridge , A. W. Stephens , J. R. Maund , S. Mattila

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

We present the results of a 10.5 yr, volume limited (28 Mpc) search for supernova (SN) progenitor stars. We compile all SNe discovered within this volume (132, of which 27% are type Ia) and determine the relative rates of each sub-type from…

天体物理学 · 物理学 2009-11-13 S. J. Smartt , J. J. Eldridge , R. M. Crockett , J. R. Maund

We present pre-explosion photometry of the likely progenitor star of the Type II supernova (SN II) 2017eaw in NGC 6946. We use a Hubble Space Telescope (HST) image of SN 2017eaw to perform relative astrometry with HST and Spitzer Space…

太阳与恒星天体物理 · 物理学 2018-09-12 Charles D. Kilpatrick , Ryan J. Foley

Linkage between core-collapse supernovae (SNe) and their progenitors is not fully understood and ongoing effort of searching and identifying the progenitors is needed. $\mathrm{SN\,2024abfl}$ is a recent Type II supernova exploded in the…

Using images from the Hubble Space Telescope (HST) and the Gemini Telescope we confirm the disappearance of the progenitors of two Type II supernovae (SNe), and evaluate the presence of other stars associated with them. We find that the…

太阳与恒星天体物理 · 物理学 2010-01-07 Justyn R. Maund , Stephen J. Smartt

We report on the direct detection and characterization of the probable red supergiant progenitor of the intermediate-luminosity Type II-Plateau (II-P) supernova (SN) 2012aw in the nearby (10.0 Mpc) spiral galaxy Messier 95 (M95; NGC 3351).…

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