Loss of Mass in Binary Systems

Details Loss of Mass in Binary Systems Loss of Mass in Binary Systems

Apr 1934

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1934natur.133r.613b&link_type=abstract

Nature, Volume 133, Issue 3364, pp. 613 (1934).

Computer Science

3

Scientific paper

SOME years ago, Sir James Jeans1 considered the problem of the variation in the orbital elements of a binary star in which one or both of the components is losing mass by radiation. He concluded that, in these circumstances, the orbital eccentricity will remain constant, whereas the semi-axis major varies inversely as the sum of the masses of the components.

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