Evolution and final fate of massive post-common-envelope binaries

Mergers of neutron stars (NSs) and black holes (BHs) are nowadays observed routinely thanks to gravitational-wave (GW) astronomy. In the isolated binary-evolution channel, a common-envelope (CE) phase of a red supergiant (RSG) and a compact object is crucial to sufficiently shrink the orbit and ther...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2024-08, Vol.688, p.A87
Hauptverfasser:	Wei, Dandan, Schneider, Fabian R. N., Podsiadlowski, Philipp, Laplace, Eva, Röpke, Friedrich K., Vetter, Marco
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Angular momentum Astronomy Binary stars Black holes Companion stars Emission Gamma ray bursts Gravitational waves Mass transfer Neutron stars Neutrons Red giant stars Resonant interactions Simulation Stellar envelopes Stellar evolution Stellar system evolution Supergiant stars Transients (astronomy)
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