V3908 Sagitarii / V3908 Sgr
Light curve obtained from 102 unfiltered images taken with the Bradford Robotic Telescope Cluster Camera between 2012 July 9 and 2015 October 29.
Photometry performed in AIP4WIN. The results have not been transformed.
This Mira type star is in the field of W Ser (see W Ser page on this site).
The period derived from my observations over a small number of cycles is 282.5 days, which compares with 279 d (GCVS) and 279.5 d (AAVSO VSX)
Photometry performed in AIP4WIN. The results have not been transformed.
This Mira type star is in the field of W Ser (see W Ser page on this site).
The period derived from my observations over a small number of cycles is 282.5 days, which compares with 279 d (GCVS) and 279.5 d (AAVSO VSX)