TIDAL SHEAR AND THE V1309 SCO MERGER
We show that the observed decline in the orbital period of the merger candidate V1309 Sco could have been driven by tidal shear energy dissipation, E˙ S. This mechanism becomes relevant once the expanding layers of an evolving star rotate asynchronously. For a 1 M⊙ + 0 . 8 M⊙ system with orbital per...
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| Veröffentlicht in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hauptverfasser: | , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
Universidad Nacional Autónoma de México
2016
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| Schlagworte: | |
| Online-Zugang: | https://www.redalyc.org/articulo.oa?id=57146052008 |
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