Minimum projection in eccentric binary orbits

Details Minimum projection in eccentric binary orbits Minimum projection in eccentric binary orbits

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....79..204m&link_type=abstract

Astronomy and Astrophysics, vol. 79, no. 1-2, Oct. 1979, p. 204-209. Research supported by the Consiglio Nazionale delle Ricerc

Astronomy and Astrophysics

Astrophysics

3

Eccentric Orbits, Eclipsing Binary Stars, Orbit Calculation, Stellar Motions, Companion Stars, Elliptical Orbits, Minima, Pulsars

Scientific paper

The minimum projected distance of the components of a binary system is calculated for any eccentricity. The idea that minimum projected distances should occur at conjunction, irrespective of eccentricity, is incorrect. A new recursive method for computing the minimum projected separation for arbitrary periastron distance has been devised and is applied to the high eccentric orbit of the binary pulsar PSR 1913 + 16.

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