44 Tau: a slowly rotating delta Scuti star

Details 44 Tau: a slowly rotating delta Scuti star 44 Tau: a slowly rotating delta Scuti star

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..256..179a&link_type=abstract

Observational Aspects of Pulsating B- and A Stars, ASP Conference Proceedings, Vol. 256. Edited by Christiaan Sterken and Donal

Astronomy and Astrophysics

Astronomy

Scientific paper

Three separate data sets of the delta Scuti star 44 Tau (HD26322), collected at the following Observatories: Washington Camp (Arizona), Sierra Nevada Observatory (Spain) and at the Ege University Observatory (Turkey), were combined and analyzed to determine its pulsation behavior. Seventeen frequencies between 6.34/d and 23.034/d (73.2 microHz and 266 microHz) were detected, of which seven are linear combinations. Furthermore, we could confirm the results of Akan (1993).

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