Improved elements for the dwarf cepheid V567 Oph.

Details Improved elements for the dwarf cepheid V567 Oph. Improved elements for the dwarf cepheid V567 Oph.

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984geocr...5.....l&link_type=abstract

GEOS Circular on RR Lyr Type Variables, No. RR 5, 5 p. (1984)

Physics

Dwarf Cepheids:Periods

Scientific paper

V567 Oph is a dwarf cepheid variable star. The period of which, given in the GCVS (1976), is 0.149521 day. The visual estimates made by GEOS observers from 1977 to 1982 enable the period to be improved. The new elements for maximum are: Max = hel JD 2,443,525.0444(+/-25) + 0.14952377(+/-13) E. The mean light curve obtained from published photoelectric measurements gives a rising branch equal to 0.31 time the period.

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