MgII-K line fluxes in cool active and quiet stars (Cardini+, 2005)

Details MgII-K line fluxes in cool active and quiet stars (Cardini+, 2005) MgII-K line fluxes in cool active and quiet stars (Cardini+, 2005)

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34300303c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/430/303. Originally published in: 2005A&A...430..303C

Physics

Stars: Late-Type, Ultraviolet, Line Profiles

Scientific paper

The data base used in the present paper was generated starting from the original sample of 230 normal stars used in a study of the Wilson-Bappu effect by Cassatella et al. (2001, Cat. , Paper I). It was a sample of stars with good quality MgII observations from IUE (see Sect. 3) and known parallaxes from HIPPARCOS with luminosity classes ranging from I to V. The resulting sample (225 stars) consists of an accurately selected, uniformly reduced and homogeneously calibrated data set.
(3 data files).

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