The Blue Supergiant Problem and the Main-Sequence Width
Using Gaia DR3 we derive new distances and luminosities for a sample of Galactic B supergiants which were thought to be post main-sequence (MS) objects from their HR diagram location beyond the terminal-age MS (TAMS). When applying the newer Gaia distances in addition to enhanced amounts of core-bou...
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| Autors principals: | , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
MDPI AG
2025-03-01
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| Col·lecció: | Galaxies |
| Matèries: | |
| Accés en línia: | https://www.mdpi.com/2075-4434/13/2/19 |
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