An astrometric study of the eclipsing binary 31 o2 cygni

Details An astrometric study of the eclipsing binary 31 o2 cygni An astrometric study of the eclipsing binary 31 o2 cygni

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phdt.........3b&link_type=abstract

Ph.D. Thesis Pittsburgh Univ., PA.

Astronomy and Astrophysics

Astronomy

1

Astrometry, Cygnus Constellation, Eclipsing Binary Stars, Stellar Spectra, Stellar Structure, Computer Programs, Data Reduction, Orbits, Stellar Mass, Stellar Spectrophotometry, Telescopes

Scientific paper

The astrometric and spectroscopic orbits of 31 o2 Cygni were studied to derive the distance, masses, and luminosities of the components. The theory of visual, astrometric, and spectroscopic orbital solutions is discussed and a rigorous method of combining such data while introducing no spurious accelerations is presented, as well as the data, computer programs, and reductions.

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