On the evolution of angular momentum, magnetic activity and mass loss rate of late type main sequence stars
With the best data, I find that nearly all 0.5 to 1.2 M main sequence stars converge to a single rotational mass-dependent sequence after 750 Myr; when M > 0.8 Mʘ , most of them converge in 120 Myr. If stars rotate as rigid bodies, most have angular momenta within clear bounds. The lower bound defin...
I tiakina i:
| I whakaputaina i: | Revista Mexicana de Astronomía y Astrofísica |
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| Kaituhi matua: | |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad Nacional Autónoma de México
2020
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| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=57171642014 https://www.redalyc.org/journal/571/57171642014/ https://www.redalyc.org/journal/571/57171642014/html/ https://www.redalyc.org/journal/571/57171642014/57171642014.epub https://www.redalyc.org/journal/571/57171642014/movil |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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