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...
保存先:
| 主要な著者: | , |
|---|---|
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
MDPI AG
2025-03-01
|
| シリーズ: | Galaxies |
| 主題: | |
| オンライン･アクセス: | https://www.mdpi.com/2075-4434/13/2/19 |
| タグ: |
タグなし, このレコードへの初めてのタグを付けませんか!
|