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Analysis of the Mg II h spectral line shapes in HR 7275 and IM Peg.
Bibcode: 1995POBeo..50..111P

Popović, L. Č.; Jankov, S.; Djurašević, G. +3 more

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.

1995 Publications de l'Observatoire Astronomique de Beograd
IUE 0