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 <...
Kaydedildi:
| Asıl Yazarlar: | , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
MDPI AG
2023-06-01
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| Seri Bilgileri: | Galaxies |
| Konular: | |
| Online Erişim: | https://www.mdpi.com/2075-4434/11/3/76 |
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