Computer Science
Scientific paper
Jun 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..31770131r&link_type=abstract
VizieR On-line Data Catalog: J/A+A/177/131. Originally published in: 1987A&A...177..131R
Computer Science
Stars: Late-Type, Stars: Dwarfs, Stars: Giant, Magnitudes: Absolute
Scientific paper
The relation between the CaII H and K line-tore flux density and rotation period is studied for a sample of 313 cool stars of luminosity classes ranging from II-III to V, and compared to similar relations for MgII h and k and soft X-ray.
(3 data files).
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