The “Canonical” White Dwarf Cooling Sequence of M5
Recently, slowly cooling white dwarfs (WDs) are a new class of WD that have been identified in two globular clusters (namely M13 and NGC 6752), showing a horizontal branch (HB) morphology with an extended blue tail. The cooling rate of these WDs is reduced by stable thermonuclear hydrogen burning in...
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| Hauptverfasser: | , , , , , , , |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
IOP Publishing
2023-01-01
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| Schriftenreihe: | The Astrophysical Journal |
| Schlagworte: | |
| Online-Zugang: | https://doi.org/10.3847/1538-4357/acd173 |
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