Mass-luminosity relation of low-mass stars (Malkov+ 1997)

Details Mass-luminosity relation of low-mass stars (Malkov+ 1997) Mass-luminosity relation of low-mass stars (Malkov+ 1997)

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..33200079m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/320/79. Originally published in: 1997A&A...320...79M

Computer Science

Stars: Late-Type, Stars: Masses

Scientific paper

To construct the MLR, empirical data for 56 stars in 30 low mass multiple systems, main sequence components of spectral class M0 and later were collected and processed. We considered only those systems where the determination of dynamical masses of components is possible, that is, where masses are derived directly from celestial mechanical considerations rather than from relations between mass and some observational parameter. (3 data files).

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