Published September 26, 2023
| Version v1
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Evidence for sub-Chandrasekhar-mass progenitors of Type Ia supernovae at the faint end of the width-luminosity relation
- 1. Laboratoire d'Astrophysique de Marseille
- 2. Institut d'Astrophysique de Paris
- 3. University of Pittsburgh
- 4. University of Chicago
Description
Hydrodynamical inputs and synthetic spectra for the complete DDC, SCH, and PDDEL model series published in Blondin et al. (2017), MNRAS, 470, 157.
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Additional details
Related works
- Cites
- Journal article: https://ui.adsabs.harvard.edu/link_gateway/2017MNRAS.470..157B/doi:10.1093/mnras/stw2492 (URL)
- Is cited by
- Preprint: 10.48550/arXiv.2309.10054 (DOI)
References
- Blondin et al. (2017), arXiv:1706.01901
- Pearson et al. (2023), arXiv:2309.10054