The Gothard Observatory Synthetic Stellar Photometry Database
Context. To determine stellar luminosities and radii, it is necessary to know the total bolometric fluxes emitted by stars - or equivalently their bolometric corrections (BCs) - as accurately as possible. Aims. The aim of this paper is to present and describe a new database of synthetic stellar magn...
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| Principais autores: | , , , , , , , , |
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| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
EDP Sciences
2026-02-01
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| Serier: | Astronomy & Astrophysics |
| Fag: | |
| Online adgang: | https://www.aanda.org/articles/aa/full_html/2026/02/aa57685-25/aa57685-25.html |
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