On (dot{m}-dot{P}) and (dot{J}-dot{P})-Type Relations for Close Binaries

Details On (dot{m}-dot{P}) and (dot{J}-dot{P})-Type Relations for Close Binaries On (dot{m}-dot{P}) and (dot{J}-dot{P})-Type Relations for Close Binaries

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.304..113k&link_type=abstract

Astrophysics and Space Science, Volume 304, Issue 1-4, pp. 113-115

Astronomy and Astrophysics

Astrophysics

3

Binary Stars, Close Binary Evolution, Physical Processes, Mass Transfer

Scientific paper

In this study we develop relations connecting the rate of orbital period variations dot{P} of binary stars with the significant parameters of their evolution, under non-conservative conditions in a fundamental level of description. In this framework, a new generalized dot{J}-dot{P}-type relation is derived, that can be used in estimation of parameters connected with basic evolutionary processes, when dot{P} is known from O-C time-series analysis.

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