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Supernova Progenitors Observed with HST

Van Dyk, Schuyler D. (2017) Supernova Progenitors Observed with HST. In: Handbook of Supernovae. Springer , Cham, Switzerland, pp. 693-719. ISBN 978-3-319-20794-0. http://resolver.caltech.edu/CaltechAUTHORS:20170718-105824395

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Abstract

To understand the relevance of supernovae and to enable their use as probes of stellar evolution throughout time, it is necessary to determine their stellar origins. I describe the direct identification of supernova progenitors in existing pre-explosion images, particularly those obtained through serendipitous imaging of nearby galaxies by the Hubble Space Telescope. Establishing the astrometric coincidence of a supernova with its putative progenitor is straightforward. The interpretation of these results is more complicated and fraught with larger uncertainties. I describe the necessary ingredients for this interpretation. I comment on specific cases, particularly for core-collapse supernova progenitors, which are the only ones that have been detected to date. I also describe the need to revisit the supernova site, long after the supernova has faded, to confirm the progenitor identification through the star’s disappearance and potentially to detect a putative binary companion that may have survived the explosion.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://dx.doi.org/10.1007/978-3-319-20794-0_126-1DOIArticle
https://link.springer.com/referenceworkentry/10.1007%2F978-3-319-20794-0_126-1PublisherArticle
ORCID:
AuthorORCID
Van Dyk, Schuyler D.0000-0001-9038-9950
Additional Information:© 2016 Springer International Publishing AG.
Group:Infrared Processing and Analysis Center (IPAC)
Record Number:CaltechAUTHORS:20170718-105824395
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170718-105824395
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:79154
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:18 Jul 2017 18:04
Last Modified:27 Nov 2017 17:30

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