Orbital inclination and mass of the binary pulsar PSR0655 + 64

Details Orbital inclination and mass of the binary pulsar PSR0655 + 64 Orbital inclination and mass of the binary pulsar PSR0655 + 64

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.310..300l&link_type=abstract

Nature (ISSN 0028-0836), vol. 310, July 26, 1984, p. 300-302.

Computer Science

27

Binary Stars, Pulsars, Stellar Mass, Companion Stars, Electron Density (Concentration), Inclination, Orbital Elements, Scintillation

Scientific paper

The author reports here variations in the rate of interstellar scintillation that have been measured as the pulsar PSR 0655+64 moves around its orbit, allowing a direct determination of the inclination of the orbit, the transverse velocity of the whole binary system through space and also of the linear scale of the interstellar scintillation pattern. The observations also provide an upper limit to the diameter of the companion star and the electron density within the orbit.

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