Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.104..133t&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 104, no. 1, Sept. 1984, p. 133-143.
Astronomy and Astrophysics
Astrophysics
7
Angular Momentum, Binary Stars, Kepler Laws, Stellar Mass, Orbital Elements, Statistical Correlation, Stellar Evolution
Scientific paper
The spectroscopic binaries, considered as a single data point, fall roughly on the 'universal' power-law of index 1.8 for angular momentum vs total mass, as defined by planets, spiral galaxies, and numerous other objects. But the individual systems in the Seventh Catalogue of the Orbital Elements of Spectroscopic Binary Systems define a curve of rather shallower slope, 1.63 + or - 0.007, over more than two orders of magnitude in mass and four in angular momentum. Various subsets (long and short periods; single and double line systems; known and unknown orbital orientations) all yield slopes from 1.48 to 1.77. These values, as well as the slightly larger one found for eclipsing systems by Sistero and Marton, are very much what one would expect, given the form of Kepler's Third Law and the stellar mass-radius relation. If only these well-known pieces of physics are at work, then the still-wider visual binaries should yield a slope near 5/3. Catalogs currently in press will permit easy testing of this prediction. It seems unlikely that deep clues to the origin of either binary systems or angular momentum are to be found from considerations of this nature.
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