Electron densities in late-type stars

Details Electron densities in late-type stars Electron densities in late-type stars

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...197..205b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 197, no. 1-2, May 1988, p. 205-208.

Astronomy and Astrophysics

Astrophysics

8

Chromosphere, Electron Density (Concentration), Giant Stars, Late Stars, Line Spectra, Supergiant Stars, Electron Impact, Fine Structure, Iue, Plasma Diagnostics, Solar Corona, Stellar Atmospheres

Scientific paper

Recently published atomic calculations for the C II UV 0.01 intersystem multiplet at 2325 Å are combined with dearchived IUE data on a number of late-type giants and supergiants to derive the electron densities in these stars' upper chromospheres/lower transition regions. The results represent a substantial change from previously derived values. The implications of this change are briefly discussed.

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