The coolest extremely low-mass white dwarfs
<i>Context.</i> Extremely low-mass white dwarf (ELM WD; M⁎ ≲ 0.18-0.20 M⊙) stars are thought to be formed in binary systems via stable or unstable mass transfer. Although stable mass transfer predicts the formation of ELM WDs with thick hydrogen (H) envelopes that are characterized by do...
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| Autores principales: | Calcaferro, Leila Magdalena, Althaus, Leandro Gabriel, Córsico, Alejandro Hugo |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93860 https://www.aanda.org/10.1051/0004-6361/201732551 https://ri.conicet.gov.ar/handle/11336/82883 |
| Aporte de: |
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