Binary Central Stars of Planetary Nebulae
It is now clear that a vast majority of intermediate-mass stars have stellar and/or sub-stellar companions, therefore it is no longer appropriate to consider planetary nebulae as a single-star phenomenon, although some single, isolated stars may well lead to planetary nebulae. As such, while underst...
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| Auteur principal: | |
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| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
MDPI AG
2020-04-01
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| Collection: | Galaxies |
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| Accès en ligne: | https://www.mdpi.com/2075-4434/8/2/28 |
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