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Evidence for stellar chromospheres in globular clusters
Published online by Cambridge University Press: 04 August 2017
Abstract
We suggest that the conspicuous gaps frequently seen in the color-magnitude diagrams of globular clusters are caused by a sudden increase in chromospheric activity shortly after stars evolve away from the main sequence.
- Type
- Stellar Coronae: Chromospheres of Cool Stars
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 357 - 358
- Copyright
- Copyright © Reidel 1987