CoBiToM Project -- II: Evolution of contact binary systems close to the orbital period cut-off

Ultra-short orbital period contact binaries (Porb < 0.26 d) host some of the smallest and least massive stars. These systems are faint and rare, and it is believed that they have reached a contact configuration after several Gyrs of evolution via angular momentum loss, mass transfer and mass loss...

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Veröffentlicht in:	arXiv.org 2021-12
Hauptverfasser:	Loukaidou, G A, Gazeas, K D, Palafouta, S, Athanasopoulos, D, Zola, S, Liakos, A, Niarchos, P G, Hakala, P, Essam, A, Hatzidimitrio, D
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular momentum Binary stars Contact angle Light curve Main sequence stars Mass transfer Massive stars Novae Orbital stability Orbits Physics - Solar and Stellar Astrophysics Stellar evolution Stellar system evolution Stellar winds
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