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Habitable Planets Around White and Brown Dwarfs: The Perils of a Cooling Primary
White and brown dwarfs are astrophysical objects that are bright enough to support an insolation habitable zone (IHZ). Unlike hydrogen-burning stars, they cool and become less luminous with time; hence their IHZ moves in with time. The inner edge of the IHZ is defined as the orbital radius at which...
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| Main Authors: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
Mary Ann Liebert, Inc.
2013
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| Assuntos: | |
| Acceso en liña: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3612282/ https://ncbi.nlm.nih.gov/pubmed/23537137 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1089/ast.2012.0867 |
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