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MK Classification and Dynamical Masses for Late‐Type Visual Binaries
2006
Publications of the Astronomical Society of the Pacific
On the basis of slit spectra obtained with the SCORPIO spectral camera attached to the 2.6 m telescope of the V. Ambartsumian Byurakan Astrophysical Observatory (Armenia), MK classifications for 30 visual binaries comprising mostly late K and M type stars are presented. Comparison with other determinations shows that this configuration provides a reliable MK classification. Dynamical masses for 25 systems are computed. Using standard mass-luminosity calibrations, individual mass sums for 11
doi:10.1086/504881
fatcat:476p2nf5lrhu3l2o54mbmypymu