Exploring massive star early evolution: the case of the Herschel 36 A triple system

ABSTRACT Theoretical models show that some massive stars have not yet arrived at the zero-age main sequence (ZAMS) at the end of the accretion phase. At that time, they have lost their thick envelopes and thus could be optically visible. Although some candidates to optically observable ZAMS stars ha...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2024-11, Vol.535 (1), p.359-369
Hauptverfasser:	Arias, Julia I, Holgado, Gonzalo, Gamen, Roberto, Morrell, Nidia I, Campillay, Abdo R
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Massive stars Pre-main sequence stars Spectrum analysis Star & galaxy formation Star formation Stellar age Stellar envelopes Stellar evolution Systems theory
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