Orbital inclination and masses newly determined from the triple system Algol

Details Orbital inclination and masses newly determined from the triple system Algol Orbital inclination and masses newly determined from the triple system Algol

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....80l..11b&link_type=abstract

Astronomy and Astrophysics, vol. 80, no. 2, Dec. 1979, p. L11, L12.

Astronomy and Astrophysics

Astrophysics

21

Algol, Interferometry, Orbital Elements, Speckle Patterns, Stellar Mass, Stellar Motions, Astrometry, Astronomical Spectroscopy, Eclipsing Binary Stars, Stellar Spectrophotometry

Scientific paper

Ten Speckle Interferometric observations of the triple system Algol are combined with spectroscopic orbital parameters for a determination of orbital inclination, the stellar masses and the distance of the system. The results confirm that the long period system Algol AB-C is nearly coplanar with the eclipsing binary Algol AB. The masses of Algol AB and Algol C derived from interferometric observations agree well with recent determination from spectroscopic studies. The new determination of the distance is consistent with the value of the trigonometric parallax.

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