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Evolution of rotating 25 M⊙ Population III star: physical properties and resulting supernovae.
- Source :
-
Monthly Notices of the Royal Astronomical Society: Letters . May2023, Vol. 521 Issue 1, pL17-L23. 7p. - Publication Year :
- 2023
-
Abstract
- In this letter, we report the outcomes of 1D modelling of a rotating 25 M⊙ zero-age main sequence Population III (Pop III) star up to the stage of the onset of core collapse. Rapidly rotating models display violent and sporadic mass-losses after the main-sequence stage. In comparison to the solar metallicity model, Pop III models show very small pre-supernova radii. Further, with models at the stage of the onset of core collapse, we simulate the hydrodynamic simulations of resulting supernovae. Depending upon the mass-losses due to corresponding rotations and stellar winds, the resulting supernovae span a class from weak Type II to Type Ib/c. We find that the absolute magnitudes of the core-collapse supernovae resulting from Pop III stars are much fainter than that resulting from a solar metallicity star. From our simulation results, we also conclude that within the considered limits of explosion energies and nickel masses, these transient events are very faint, making it difficult for them to be detected at high-redshifts. [ABSTRACT FROM AUTHOR]
- Subjects :
- *SUPERNOVAE
*STELLAR winds
*STELLAR populations
*STELLAR rotation
*FLAMMABLE limits
Subjects
Details
- Language :
- English
- ISSN :
- 17453925
- Volume :
- 521
- Issue :
- 1
- Database :
- Academic Search Index
- Journal :
- Monthly Notices of the Royal Astronomical Society: Letters
- Publication Type :
- Academic Journal
- Accession number :
- 162589079
- Full Text :
- https://doi.org/10.1093/mnrasl/slad020