A photometric study of the Algol system Y Hydri

Details A photometric study of the Algol system Y Hydri A photometric study of the Algol system Y Hydri

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..345d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 119, no. 2, Feb. 1986, p. 345-352. Sponsorship: Ministry of Education, Sci

Astronomy and Astrophysics

Astrophysics

Eclipsing Binary Stars, Spectrum Analysis, Stellar Spectrophotometry, Light Curve, Stellar Occultation, Tables (Data), Ubv Spectra

Scientific paper

A synthetic light curve technique is used to analyze 50-cm 297-UBV
observations of the Algol-type eclipsing binary Y Hyi obtained in 1976
and 1977. The system shows complete eclipses, and is semi-detached, with
the secondary filling its critical Roche lobe. The primary minimum is
due to an occultation.

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