Densities, Temperatures and Geometric Extents of C II Emitting Regions in the Winds of Luminous, Late-Type Stars

Details Densities, Temperatures and Geometric Extents of C II Emitting Regions in the Winds of Luminous, Late-Type Stars Densities, Temperatures and Geometric Extents of C II Emitting Regions in the Winds of Luminous, Late-Type Stars

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mlrg.proc...55c&link_type=abstract

Mass Loss from Red Giants; Proceedings of the Conference, University of California, Los Angeles, CA, June 20, 21, 1984. Edited

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

The authors summarize techniques for using IUE observations of the C II UV 0.01 and UV 1 emission line multiplets at 2325 Å and 1335 Å to estimate the electron density (Ne) and temperature (Te) in, and the geometric extent of, the chromospheres of late-type stars. The results of applying these techniques to a sample of 15 stars observed with the IUE satellite are discussed.

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