Light curve analysis of 44 Tauri

Details Light curve analysis of 44 Tauri Light curve analysis of 44 Tauri

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993dssn....6...11a&link_type=abstract

Delta Scuti Star Newsletter, Issue 6, p. 11-13.

Physics

1

Scientific paper

Two separate sets of data obtained at Merate (Poretti et al. 1992) and Ege University Observatories were combined and analyzed by means of the program PERIOD (Breger, 1990) in order to monitor the star's pulsational behaviour. The present data have been obtained on 12 nights (three nights on December 1 989, two nights on November 1990, six nights on January 1991 and one night on February 1991), being mostly crowded around January 1991 which is separated by roughly one year from the Poretti et al. data. The analysis led to a seven-frequency solution (Table 1) and gave a clue that 44 Tau might have experienced some variations in its pulsational behaviour within a one-year period.

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