Abstract
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.
| Original language | English |
|---|---|
| Title of host publication | Living Around Active Stars |
| Subtitle of host publication | Proceedings of the International Astronomical Union, IAU Symposium |
| Editors | Didyendu Nandy, Adriana Valio, Pascal Petit |
| Publisher | Cambridge University Press |
| Pages | 252-263 |
| Number of pages | 11 |
| Volume | 328 |
| ISBN (Print) | 9781107170056 |
| DOIs | |
| Publication status | Published - Oct 2017 |
Keywords
- stars: activity
- stars: chromospheres
- stars: coronae
- stars: evolution
- stars: interiors
- stars: late-type
- stars: magnetic fields
- stars: pre-main sequence
- stars: rotation
- X-rays: stars