On the possible multiplicity of the components of some low-mass systems

Details On the possible multiplicity of the components of some low-mass systems On the possible multiplicity of the components of some low-mass systems

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43...80k&link_type=abstract

Astronomy Reports, Volume 43, Issue 2, February 1999, pp.80-88

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Multiplicity is one factor that can displace a star from the standard mass-luminosity relationship. Assuming that the components of some low-mass systems whose mass is higher than expected are unresolved binaries, we have calculated the most probable values for the masses and luminosities of the hidden components. The calculations are based on a technique for the minimization of a function of many variables.

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