Analysis of the Mg II h spectral line shapes in HR 7275 and IM Peg.

Details Analysis of the Mg II h spectral line shapes in HR 7275 and IM Peg. Analysis of the Mg II h spectral line shapes in HR 7275 and IM Peg.

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pobeo..50..111p&link_type=abstract

Publications de l'Observatoire Astronomique de Beograd, No. 50, p. 111 - 114

Astronomy and Astrophysics

Astronomy

Uv Spectra: Rs Cvn Stars, Interstellar Absorption: Stellar Spectra

Scientific paper

The analysis of high-resolution IUE spectra of the RS CVn type stars HR
7275 and IM Peg is presented. The inverse method technique was applied
to the Mg II h chromospheric emission line, that shows the presence of
interstellar absorption, in order to recover the intrinsic stellar line
profile parameters.

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