The chromospheric activity, kinematics and metallicities of gliese catalog M dwarfs
We have obtained a large body of photometry and echelle spectra for a set of stars composed of all Gliese catalog M dwarfs north of -10° and brighter than 12th magnitude. A paper reviewing the results of the M dwarf program will appear shortly (Stauffer and Hartmann 1985). Here we will outline a few of our conclusions.
KeywordsEquivalent Width Star Formation Rate Space Motion Metal Poor Star Echelle Spectrograph
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