Orbital Period Changes in Recurrent Nova T Corona Borealis Prove That It Is Not a Type Ia Supernovae Progenitor
T Corona Borealis (T CrB) is a recurrent nova and a symbiotic star that is commonly highlighted as the best case for being a progenitor of a Type Ia supernova (SN Ia) within the framework of single-degenerate models. This exemplar can be tested by measuring whether the white dwarf (WD) mass ( M _WD...
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| Format: | Artigo |
| Jezik: | Inglês |
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IOP Publishing
2025-01-01
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| Serija: | The Astrophysical Journal |
| Teme: | |
| Online dostop: | https://doi.org/10.3847/1538-4357/adfa16 |
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