Dense Molecular Environments of B[e] Supergiants and Yellow Hypergiants

Dense Molecular Environments of B[e] Supergiants and Yellow Hypergiants

Massive stars expel large amounts of mass during their late evolutionary phases. We aim to unveil the physical conditions within the warm molecular environments of B[e] supergiants (B[e]SGs) and yellow hypergiants (YHGs), which are known to be embedded in circumstellar shells and disks. We present &...

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Bibliographic Details
Main Authors: Michaela Kraus, Michalis Kourniotis, María Laura Arias, Andrea F. Torres, Dieter H. Nickeler
Format: Article
Language:English
Published: MDPI AG 2023-06-01
Series:Galaxies
Subjects:
stars: massive
stars: supergiants
stars: winds
outflows
circumstellar matter
Online Access:https://www.mdpi.com/2075-4434/11/3/76

Internet

https://www.mdpi.com/2075-4434/11/3/76

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