Improvement of the period for the RR Lyr star TZ Aurigae.

Details Improvement of the period for the RR Lyr star TZ Aurigae. Improvement of the period for the RR Lyr star TZ Aurigae.

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993geocr..12.....b&link_type=abstract

GEOS Circular on RR Lyr Type Variables, No. RR 12, 7 p. (1993)

Computer Science

Scientific paper

From the times of maximum light published by Tsesevitch, and those
obtained visually by members of the GEOS and the BAV, an ephemeris can
be computed: Max (J.D.Hel) = 2,419,902.4287(+/-18) + 0.391674800(+/-
77)*E. This confirms that the period of TZ Aur has not significantly
changed over an interval of more than 70,000 cycles.

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