The long-term evolution of stellar activity

The long-term evolution of stellar activity

I review the evolution of low-mass stars with outer convective zones over timescales of millions-to-billions of years, from the pre-main sequence to solar-age, ~4.6 Gyr (Bahcall et al. 1995; Amelin et al. 2010), and beyond. I discuss the evolution of high-energy coronal and chromospheric emission, t...

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Veröffentlicht in:Proceedings of the International Astronomical Union 2016-10, Vol.12 (S328), p.252-263
1. Verfasser: Gregory, Scott G.
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Contributed Papers
Coronas
Magnetism
Pre-main sequence stars
Stellar activity
Stellar evolution
Stellar rotation
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Zusammenfassung:I review the evolution of low-mass stars with outer convective zones over timescales of millions-to-billions of years, from the pre-main sequence to solar-age, ~4.6 Gyr (Bahcall et al. 1995; Amelin et al. 2010), and beyond. I discuss the evolution of high-energy coronal and chromospheric emission, the links with stellar rotation and magnetism, and the emergence of the rotation-activity relation for stars within young clusters.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921317003891