BV observations of the eclipsing binary WX Eridani

Details BV observations of the eclipsing binary WX Eridani BV observations of the eclipsing binary WX Eridani

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.121..301s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 121, no. 2, April 1986, p. 301-308.

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Electrophotometry, Stellar Spectrophotometry, Ubv Spectra, Spectrum Analysis, Stellar Color, Stellar Magnitude

Scientific paper

Photoelectric observations of WX Eri made on the 56-cm Uttar Pradesh State Observatory telescope through B and V filters, are discussed. The magnitudes of the system at maximum are B = 9.70m and V = 9.46m. The primary component has a B - V color of 0.16m, and is found to have a spectral type of A5. The secondary component has a B - V color of 0.80m and a spectral type of KO. The period is found to be constant and is calculated to be 0.82327076d. No delta-Scuti type light variations were noticed during observations made near the maximum phase.

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