Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..219..935w&link_type=abstract
Stars as suns : activity, evolution and planets, Proceedings of the 219th symposium of the International Astronomical Union held
Astronomy and Astrophysics
Astronomy
Scientific paper
We present a study of the magnetic activity properties of low-mass stars in the Sloan Digital Sky Survey. Using the H-alpha emission line as an activity indicator we examine the fraction of active stars as a function of spectral type and find a peak near type M7 confirming previous results. However contrary to past findings we find that not all M7 stars are active. We investigate the ratio of the luminosity emitted in H-alpha compared to the bolometric luminosity for each star and find a roughly constant ratio (with large scatter) over the range M0-M7. There appears to be a slight decrease in this ratio for types M8-L0 in agreement with previous determinations. We also explore the effect of metallicity on activity and examine whether activity is correlated with changes in SDSS colors.
Covey Kevin R.
Hawley Suzanne L.
Walkowicz Lucianne M.
West Andrew A.
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