The Panchromatic Hubble Andromeda Treasury. XX. The Disk of M31 is Thick
We present a new approach to measuring the thickness of a partially face-on stellar disk, using dust geometry. In a moderately-inclined disk galaxy, the fraction of reddened stars is expected to be 50% everywhere, assuming that dust lies in a thin midplane. In a thickened disk, however, a wide range...
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| Главные авторы: | , , , , , , , , |
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| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
IOP Publishing
2023-01-01
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| Серии: | The Astronomical Journal |
| Предметы: | |
| Online-ссылка: | https://doi.org/10.3847/1538-3881/accc83 |
| Метки: |
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