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OEJV# Publication's title Author   Date
  Abstract / note  

 
0063GI Aqr Is RRab Type Star
397 kB
Petr Sobotka2007-05-16
 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.

Simbad object(s): GI Aqr,

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