Here are some observations of neglected semiregular variables near North Pole made by me and partly by Lubo Brát since Summer 2000.
| According to GCVS, AD Cep is a SR star with variations between 10.8 and 15.5 mag (pg), period of 166 days and spectrum M6.5 - M8. DFT on our observations suggests period of 167 days but there is probably a second period of 313 days which makes every second minimum deeper. Also, the range of variability is smaller. | |
| According to GCVS, FF Cep is a SRa star with period of 185 days and range of variability 10.3 - 11.2 mag (pg), spectrum M. DFT on our data suggests 190 day period, in perfect agreement with GCVS. | |
| According to GCVS, OU Cep is a SR star with range 11.1 - 12.0 (pg), unknown period and spectrum M8. DFT on our observations suggest period of 127 days. | |
| According to GCVS, CW Dra is a Lb: star with range 10.8 - 11.7 (pg) and spectrum M8. Our observations are just scatter. Further observations are needed. | |
| According to GCVS, IQ Dra is a SRb: star discovered by Hipparcos with range of 8.47 - 8.95 mag (Hp). There can be some variations in our data, but we do not believe them much. |