Different to the core: The pre-supernova structures of massive single and binary-stripped stars

The majority of massive stars live in binary or multiple systems and will interact with a companion during their lifetimes, which helps to explain the observed diversity of core-collapse supernovae. Donor stars in binary systems can lose most of their hydrogen-rich envelopes through mass transfer. A...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-12, Vol.656, p.A58
Hauptverfasser:	Laplace, E., Justham, S., Renzo, M., Götberg, Y., Farmer, R., Vartanyan, D., de Mink, S. E.
Format:	Artikel
Sprache:	eng
Schlagworte:	abundances ASTRONOMY AND ASTROPHYSICS binaries Binary stars Carbon close Companion stars evolution Helium Mass transfer massive Massive stars Metallicity Neon neutron Nuclear fusion nuclear reactions Nuclear reactors nucleosynthesis Oxygen Silicon stars Stellar evolution Supernovae Surface properties
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