Spectroscopic binaries near the north galactic pole. VI - BD 33.2206 deg

Details Spectroscopic binaries near the north galactic pole. VI - BD 33.2206 deg Spectroscopic binaries near the north galactic pole. VI - BD 33.2206 deg

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982japa....3..383g&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 3, Dec. 1982, p. 383-392.

Astronomy and Astrophysics

Astrophysics

9

Binary Stars, Eccentric Orbits, Electrophotometry, Radial Velocity, Stellar Spectra, Late Stars, Stellar Luminosity, Stellar Magnitude, Stellar Motions

Scientific paper

Photoelectric radial-velocity measurements have confirmed O. C. Wilson's finding that BD 33°2206, the secondary star in the wide visual binary ADS 8470, is a spectroscopic binary. It has an eccentric orbit with a period of 100 days. Its γ-velocity is close to the constant radial velocity of the visual primary, confirming the physical association of the stars.

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