Spectroscopic binary orbits from photoelectric radial velocities. Paper 69: HD 55510

Details Spectroscopic binary orbits from photoelectric radial velocities. Paper 69: HD 55510 Spectroscopic binary orbits from photoelectric radial velocities. Paper 69: HD 55510

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986obs...106..108g&link_type=abstract

The Observatory, vol. 106, p. 108-113 (1986)

Physics

7

Scientific paper

HD 55510, a ninth-magnitude object in Gemini, is shown to be a
double-lined spectroscopic binary system. It probably consists of two
late-type giants, and is only the seventh such system to be discovered.
The orbit is non-circular and has a period of 647 days.

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