The Spectroscopic Orbit of H.R. 6532 and the Radial Velocities of Ten Stars

Details The Spectroscopic Orbit of H.R. 6532 and the Radial Velocities of Ten Stars The Spectroscopic Orbit of H.R. 6532 and the Radial Velocities of Ten Stars

Sep 1922

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1922pdao....2..159c&link_type=abstract

Publications of the Dominion Observatory Ottawa, vol. 2, pp.159-166

Physics

2

Scientific paper

Thirty-three single-prism spectrograms of the star H.R. 6532 (alpha = 17h 27m.6, delta = 12deg 00') form the basis of the determination of its orbit. The period is 6.7984 days, the eccentricity .069 and semi-amplitude 50.18 km. Ten stars of different types were selected from the Harvard Catalogue to fill in a program and the radial velocities of these are determined. From three to eight plates of each star were measured.

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