Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf

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 future surveys to improve on progenitor detections. Here we report...

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Main Authors: Joanne L Pledger, Michael M Shara
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
Online Access:https://doi.org/10.3847/2041-8213/ace88b
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author Joanne L Pledger
Michael M Shara
author_facet Joanne L Pledger
Michael M Shara
author_sort Joanne L Pledger
collection DOAJ
description 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 future surveys to improve on progenitor detections. Here we report the serendipitous preexplosion imaging, by the Hubble Space Telescope, of SN 2023ixf, one of the nearest extragalactic supernovae ever discovered, in the galaxy M101. The extremely red color and absolute magnitude ${M}_{{\rm{F}}814{\rm{W}}}=-{5.11}_{-0.47}^{+0.65}$ mag suggest that the progenitor was a red supergiant. Comparison with stellar evolutionary isochrones suggests it is within the relatively low initial mass range of ∼8–10 M _⊙ and that there is likely a lot of dust present at the supernova site.
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spelling doaj.art-a683b7434bc54b9f8831d8ba8ae0574b2023-09-03T12:20:52ZengIOP PublishingThe Astrophysical Journal Letters2041-82052023-01-019531L1410.3847/2041-8213/ace88bPossible Detection of the Progenitor of the Type II Supernova SN 2023ixfJoanne L Pledger0https://orcid.org/0000-0001-8907-3051Michael M Shara1https://orcid.org/0000-0003-0155-2539Jeremiah Horrocks Institute, University of Central Lancashire , Preston, PR1 2HE, UK ; jpledger@uclan.ac.ukAmerican Museum of Natural History , New York City, NY 10024, USAStellar 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 future surveys to improve on progenitor detections. Here we report the serendipitous preexplosion imaging, by the Hubble Space Telescope, of SN 2023ixf, one of the nearest extragalactic supernovae ever discovered, in the galaxy M101. The extremely red color and absolute magnitude ${M}_{{\rm{F}}814{\rm{W}}}=-{5.11}_{-0.47}^{+0.65}$ mag suggest that the progenitor was a red supergiant. Comparison with stellar evolutionary isochrones suggests it is within the relatively low initial mass range of ∼8–10 M _⊙ and that there is likely a lot of dust present at the supernova site.https://doi.org/10.3847/2041-8213/ace88bType II supernovaeSupernovaeCore-collapse supernovae
spellingShingle Joanne L Pledger
Michael M Shara
Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf
The Astrophysical Journal Letters
Type II supernovae
Supernovae
Core-collapse supernovae
title Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf
title_full Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf
title_fullStr Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf
title_full_unstemmed Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf
title_short Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf
title_sort possible detection of the progenitor of the type ii supernova sn 2023ixf
topic Type II supernovae
Supernovae
Core-collapse supernovae
url https://doi.org/10.3847/2041-8213/ace88b
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