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Title: The Masses of Supernova Remnant Progenitors in M33
Abstract Using resolved optical stellar photometry from the Panchromatic Hubble Andromeda Treasury Triangulum Extended Region survey, we measured the star formation history near the position of 85 supernova remnants (SNRs) in M33. We constrained the progenitor masses for 60 of these SNRs, finding that the remaining 25 remnants had no local star formation in the last 56 Myr, consistent with core-collapse supernovae, making them potential Type Ia candidates. We then infer a progenitor mass distribution from the age distribution, assuming single star evolution. We find that the progenitor mass distribution is consistent with being drawn from a power law with an index of − 2.9 − 1.0 + 1.2 . Additionally, we infer a minimum progenitor mass of 7.1 − 0.2 + 0.1 M ⊙ from this sample, consistent with several previous studies, providing further evidence that stars with ages older than the lifetimes of single 8 M ⊙ stars are producing supernovae.  more » « less
Award ID(s):
2102721
PAR ID:
10423905
Author(s) / Creator(s):
; ; ; ; ; ; ; ; ;
Date Published:
Journal Name:
The Astrophysical Journal
Volume:
949
Issue:
1
ISSN:
0004-637X
Page Range / eLocation ID:
32
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
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