UBV light variation and orbital elements of MW Pavonis

Details UBV light variation and orbital elements of MW Pavonis UBV light variation and orbital elements of MW Pavonis

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..46..155l&link_type=abstract

Astrophysics and Space Science, vol. 46, Jan. 1977, p. 155-164.

Astronomy and Astrophysics

Astrophysics

5

Electrophotometry, Light Curve, Orbital Elements, Ubv Spectra, Variable Stars, Ephemeris Time, Reflecting Telescopes, Stellar Spectra, Stellar Spectrophotometry, Tables (Data)

Scientific paper

Photoelectric UBV observations of the W UMa-system MW Pavonis are presented; they were made at Bosque Alegre Station of Córdoba Observatory in 1972 and 1974. The period and linear ephemeris were obtained from nine times of minimum observed in each color. Satisfactory orbital elements were determined for the three light curves on the basis of the Russell model

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