Intermediate Band Photometry of V Puppis

Details Intermediate Band Photometry of V Puppis Intermediate Band Photometry of V Puppis

Jun 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971bott....6...89m&link_type=abstract

Boletín de los Observatorios de Tonantzintla y Tacubaya Vol. 6, pp. 89-94 (1971) (http://www.astroscu.unam.mx/~bott/)

Astronomy and Astrophysics

Astronomy

6

Stars: Binaries: Eclipsing

Scientific paper

Some 150 observations were made on V Puppis on the (33, 35, 37, 40, 45, 52, 58, 63)-photometric system. The obtained light curves are of high quality. The observed amplitude of the light variations for the primary minimum depends on the spectral region in which the observations are made. To the shortest wavelength corresponds the largest amplitude. Absolute visual magnitudes are derived at primary minimum and maximum light.

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