The chromospherically active solar-type spectroscopic binary HD 191262

Details The chromospherically active solar-type spectroscopic binary HD 191262 The chromospherically active solar-type spectroscopic binary HD 191262

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990japa...11...43g&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 11, March 1990, p. 43-48.

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Radial Velocity, Stellar Orbits, Astronomical Spectroscopy, Stellar Activity, Stellar Atmospheres

Scientific paper

HD 191262 is a double-lined spectroscopic binary consisting of two
slightly unequal solar-type stars in an orbit with a period of 5.43435
days. The system is both synchronized and circularized and is probably
at least as old as the sun. The inclination of the system is about 45
degrees.

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