Chromospheric-coronal activity at high saturated levels

Details Chromospheric-coronal activity at high saturated levels Chromospheric-coronal activity at high saturated levels

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.263..113v&link_type=abstract

In ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE p 113-11

Astronomy and Astrophysics

Astrophysics

6

Chromosphere, Dwarf Stars, Iue, Stellar Activity, Stellar Coronas, Magnesium, Stellar Color, Stellar Spectrophotometry, Ultraviolet Spectra

Scientific paper

The Mg II fluxes in cool dwarf stars were calculated by measuring a 4 A passband centered on the Mg II k line in high-resolution IUE spectra, and by calibrating the continuum flux using spectra of narrow-lined stars. These measurements and published data on Mg II, C IV, and X-ray emission are discussed. Qualitative physical interpretations for the upper boundaries (in the flux-color diagrams) are suggested.

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