Disappearance of coronal X-ray emission in stars with cool dense winds
- 1 November 1992
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 360 (6401) , 239-241
- https://doi.org/10.1038/360239a0
Abstract
No abstract availableKeywords
This publication has 23 references indexed in Scilit:
- ROSAT X-ray observations of hybrid starsThe Astrophysical Journal, 1992
- X-ray emission from hybrid-chromosphere starsThe Astrophysical Journal, 1991
- Mass loss mechanisms in evolved starsThe Astronomy and Astrophysics Review, 1991
- Andromedae (K3 III):an IRAS source with an unusual ultraviolet spectrum*Monthly Notices of the Royal Astronomical Society, 1987
- Mass Loss from Cool StarsAnnual Review of Astronomy and Astrophysics, 1986
- Further observational evidence for a coronal boundary line in the cool star region of the H-R diagramThe Astrophysical Journal, 1982
- On the reality of a boundary in the H-R diagram between late-type stars with and without high temperature outer atmospheresThe Astrophysical Journal, 1982
- The cool half of the H-R diagram in soft X-raysThe Astrophysical Journal, 1981
- Hybrid atmospheres and winds in supergiant starsThe Astrophysical Journal, 1980
- Outer atmospheres of cool stars. I - The sharp division into solar-type and non-solar-type starsThe Astrophysical Journal, 1979