The Mass/Eccentricity Limit in Double Star Astronomy

Details The Mass/Eccentricity Limit in Double Star Astronomy The Mass/Eccentricity Limit in Double Star Astronomy

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003japa...24...99d&link_type=abstract

Journal of Astrophysics and Astronomy, Vol. 26, Issue 2-3, p.99

Statistics

1

Stellar Evolution, Statistics, Binaries

Scientific paper

A research that we conducted in 1963 on the evolution of the binaries based on the available orbital data to obtain a philosophical degree, led to the establishment of an interesting and new diagram between the logarithm of the total mass and a particular parameter X, bound to the areal constant. This appeared to have a real physical significance but the basic observational material was insufficiently extended to assure its undeniable existence. In 1981, a new research based on a more extended orbital material, has confirmed this diagram. Presently, another important increase in the orbital material and the availability of highly accurate trigonometric parallaxes produced by the Hipparcos satellite, gave us the opportunity to confirm once more the stability of this diagram. This last research is here described.

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