Evidence for extended chromospheres surrounding red giant stars

Details Evidence for extended chromospheres surrounding red giant stars Evidence for extended chromospheres surrounding red giant stars

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982saosr.392a.137s&link_type=abstract

In Smithsonian Astrophysics Observatory 2nd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Vol. 1 p 137-145 (

Astronomy and Astrophysics

Astrophysics

9

Chromosphere, Red Giant Stars, Cool Stars, Emission Spectra, Hydrogen Ions, Stellar Mass Ejection, Stellar Spectra, Stellar Temperature, Supergiant Stars, Ultraviolet Spectroscopy

Scientific paper

There is now an increasing amount of both observational evidence and theoretical arguments that regions of partially ionized hydrogen extending several stellar radii are an important feature of red giant and supergiant stars. This evidence is discussed and the implications of the existence of extended chromospheres in terms of the nature of the outer atmospheres of, and mass loss from, cool stars are examined.

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