The astrometric binary MU Cassiopeiae - Photographically almost resolved

Details The astrometric binary MU Cassiopeiae - Photographically almost resolved The astrometric binary MU Cassiopeiae - Photographically almost resolved

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...209..497f&link_type=abstract

Astrophysical Journal, vol. 209, Oct. 15, 1976, pt. 1, p. 497-499, 501, 502.

Astronomy and Astrophysics

Astrophysics

5

Astrometry, Astronomical Photography, Binary Stars, Subdwarf Stars, Abundance, Photographic Plates, Stellar Luminosity

Scientific paper

Photographic observations of the Population II subdwarf astrometric binary Mu Cas are described which almost resolve the components and permit an estimate of their magnitudes and separation. Red- and blue-light photographs of the system were taken during an observing period when the component separation was maximum. The separation of the two components is estimated to be about 1.5 arcsec, position angles of about 194 and 201 deg are determined for the two years of the observing period, and the apparent magnitude of the faint companion is found to be approximately 10.

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