IUE observations of BY Draconis

Details IUE observations of BY Draconis IUE observations of BY Draconis

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..243b&link_type=abstract

In ESA Fourth European IUE Conf. p 243-246 (SEE N84-35135 24-88)

Other

1

Dwarf Stars, Late Stars, Stellar Flares, Stellar Spectra, Iue, Line Spectra, Ultraviolet Spectra, Variable Stars

Scientific paper

Phased IUE low resolution observations of BY Draconis are discussed. They show no significant modulation of the prominent SWP emission lines over one rotation period. However a marginally significant anticorrelation of the MgII flux, and the flux in the LWR continuum, with the V light curve is observed, and is interpreted as due to plage type areas over the photospheric spots. Two SWP spectra show sporadic enhancements of the emission lines, as seen in other IUE spectra of flares.

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