Photometry of TT ARIETIS

Details Photometry of TT ARIETIS Photometry of TT ARIETIS

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..167s&link_type=abstract

(IAU, DFG, and Bayerisches Staatsministerium für Unterricht und Kultus, Colloquium on Cataclysmic Variables, Recent Multi-Freque

Astronomy and Astrophysics

Astrophysics

5

Cataclysmic Variables, Stellar Spectrophotometry, Fourier Analysis

Scientific paper

An analysis of data spanning 24 years shows that a secondary 20m periodicity is a persistent feature in photometric observations of TT Ari. This period decreases from 27m in 1961 to 17m in 1985. The 4d beat period of 3h.2 photometric and 3h.3 spectroscopic periods is also apparent in observations of 1966.

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