Theoretical studies of chromospheres and winds in cool stars

Details Theoretical studies of chromospheres and winds in cool stars Theoretical studies of chromospheres and winds in cool stars

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sao..rept.....h&link_type=abstract

Semiannual Progress Report, 1 Apr. - 30 Sep. 1984 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astrophysics

Chromosphere, Cool Stars, Dwarf Stars, Giant Stars, H Alpha Line, M Stars, Main Sequence Stars, Stellar Atmospheres, Stellar Envelopes, Stellar Winds, Supergiant Stars, Balmer Series, Hydrogen, Photoionization, Stellar Models

Scientific paper

The atmospheres of hot pre-main sequence stars are discussed along with
FU Orionis winds, h alpha emission from M dwarfs, and envelopes of T
Tauri stars. In addition, extended chromospheres of M supergiants and
metal deficiency giants are considered.

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