Angular momenta in binary systems

Details Angular momenta in binary systems Angular momenta in binary systems

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.146...99q&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 146, no. 1, July 1988, p. 99-137. CNPq-FINEP-CAPES-supported research.

Statistics

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3

Angular Momentum, Binary Stars, Computational Astrophysics, Kepler Laws, Main Sequence Stars, Stellar Luminosity, Stellar Mass, Unified Field Theory

Scientific paper

The correlations of angular momenta L to masses M are studied for different types of spectroscopic binaries. Postulates about equivalent states of angular momenta for different orbital parameters are introduced. From comparisons with galaxies and single stars, it is evidenced that there is not a unique universal function L = AM exp b, when the finite structure of the relation is analyzed: each object has its own coefficients A, b. It seems that there are an upper and a lower limit for all the possible functions.

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