GI Aqr Is RRab Type Star

Details GI Aqr Is RRab Type Star GI Aqr Is RRab Type Star

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007oejv...63....1s&link_type=abstract

Open European Journal on Variable Stars, vol. 0063, Issue 1, p.1

Physics

Scientific paper

Observations by INTEGRAL Optical Monitoring Camera (OMC) showed, that
the GI Aqr is not an eclipsing binary of EB type as given by GCVS. Based
on CCD V-filtered observations, GI Aqr is pulsating RRab type star. To
determine new light elements also ROTSE and ASAS-3 data were used.
P=0.6097 ± 0.0003 days, T0(max) = 2451314.7593.

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