Interstellar scintillations of binary pulsars

Details Interstellar scintillations of binary pulsars Interstellar scintillations of binary pulsars

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..174..217d&link_type=abstract

IN: Radio wave scattering in the interstellar medium; Proceedings of the AIP Conference, San Diego, CA, Jan. 18, 19, 1988 (A89-2

Physics

14

Binary Stars, Interstellar Matter, Pulsars, Scintillation, Stellar Motions, Doppler Effect, Stellar Models, Stellar Orbits

Scientific paper

Interstellar scintillations of two binary pulsars (1855+09 and 1913+16) have been measured to determine their transverse velocities at numerous points in their orbits. Combining transverse velocities with radial velocities derived from Doppler shifts, it is (in principle) possible to determine a binary system's proper motion and orbital inclination, and the bulk velocity of the scattering material along the line of sight. The present observations do not permit unambiguous determination of these quantities, but place interesting limits on some of them.

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