Magnetic Activity in Low Mass Stars: SDSS Results

Astronomy and Astrophysics – Astronomy

Scientific paper

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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.

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