SS 433 - Intensive 4 month light curves

Details SS 433 - Intensive 4 month light curves SS 433 - Intensive 4 month light curves

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238l.133k&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 238, June 15, 1980, p. L133-L138. NSF-NASA-supported research.

Astronomy and Astrophysics

Astrophysics

22

Astronomical Photometry, Binary Stars, Light Curve, Stellar Spectrophotometry, Variable Stars, Power Spectra, Spectrum Analysis, Ubv Spectra

Scientific paper

Photometry covering 100 nights during 1979 July-November is reported, in an unfiltered band (effectively 5200-8000 A), in a V band, and with a few measures in B. Correlation with the 13 day period of Crampton, Cowley, and Hutchings is found in the form of a double-peaked light curve. A more tentative connection with the 164 day 'precession' period suggested by a broad light minimum near a critical phase in the long cycle is found.

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