Sd. Williams et al., SPECTROSCOPY AND PHOTOMETRY FOR LOW-MASS STARS IN PRAESEPE, Publications of the Astronomical Society of the Pacific, 106(702), 1994, pp. 817-821
Citations number
21
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Publications of the Astronomical Society of the Pacific
We have obtained spectral types, Halpha equivalent widths, and optical
photometry for a small sample of late K and M dwarf candidate members
of the Praesepe open cluster. At least for the small sample of stars
we have observed, all of the Praesepe members later than M2 have Halph
a in emission. The chromospheric activity of the Praesepe stars is ess
entially the same as that for Hyades members of the same mass, as expe
cted since the two clusters are thought to be the same age.