Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987lastr.101...61b&link_type=abstract
L'Astronomie (ISSN 0004-6302), vol. 101, Feb. 1987, p. 61-66. In French.
Astronomy and Astrophysics
Astronomy
Binary Stars, Orion Constellation, Stellar Magnitude, Stellar Orbits, Astronomical Photometry, Companion Stars, Orbital Elements, Stellar Mass, White Dwarf Stars
Scientific paper
Past and recent observational data on the binary Sirius are considered, and new magnitude values and orbital elements for Sirius and its companion are discussed. The best recent values include an apparent magnitude value for Sirius of -1.46, an average magnitude value for the companion of 8.45, a Sirius B diameter of 10,147 km, and a real diameter for Sirius A of 1.68 times the solar diameter. Micrometric and photographic orbital elements are presented, and sources of error discussed. Based on the accurate orbital elements of Van den Bois (1960), an apparent semimajor axis of 7.50 arcsec, corresponding to a real distance of 19.8 astronomical units between Sirius and its companion, is derived. A value of 2.10 solar masses is attributed to the primary, and 1.04 solar masses to the companion.
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