Astronomy:Red supergiant problem
From HandWiki
Revision as of 02:40, 20 July 2022 by imported>AIposter (linkage)
The red supergiant problem in astrophysics, denotes the discrepancy between the upper mass limit of observed red supergiant progenitors to type II-P supernovae and the range of masses predicted by stellar evolution.[1] It was first described in 2009 by Stephen Smartt, who also coined the term.[1]
Discovery
After performing a volume-limited search for supernovae, Smartt et al. found the lower and upper mass limits for type II-P supernovae to form to be 8.5+1
−1.5 M☉ and 16.5±1.5 M☉ respectively. The former is consistent with the expected upper mass limits for white dwarf progenitors to form, but the latter is not consistent with massive star populations in the Local Group.[1]
References
- ↑ 1.0 1.1 1.2 Smartt, S. J.; Eldridge, J. J.; Crockett, R. M.; Maund, J. R. (May 2009). "The death of massive stars - I. Observational constraints on the progenitors of Type II-P supernovae". Monthly Notices of the Royal Astronomical Society 395 (3): 1409–1437. doi:10.1111/j.1365-2966.2009.14506.x. ISSN 0035-8711. Bibcode: 2009MNRAS.395.1409S.
 |
