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## (from tabmap V6.0 (2016-08-18)) 2024-04-19T06:48:09 #--------------------------------------------------------------------------- #-- J/AcA/58/279 Moscow Digital Variables in Field of 66 Oph (Kolesnikova+, 2008) #-------------------------------------------------------------------------- #---Table: J/AcA/58/279/./remarks.dat Remarks on variable stars (47 records) # Rem I2 --- Remark number # Text A66 --- Text of the remark --------------------------------------------------------------------- R| em|Text --|------------------------------------------------------------------ 1| Variable in NSVS data. 2| P=55.6d (from NSVS data). 3| A twice shorter period and type RRC are possible. 4| P=39.7d (NSVS data). 5| A small-amplitude variable in NSVS data. 6| P=60d (NSVS data). 7| P~50d (NSVS data) is possible. 8| A twice longer period is possible. 9| A twice longer period and type EW are possible. 10| P~51d (NSVS data) is possible. 11| A CCD study following this discovery was announced in 11| Antipin et al. (2007PZ.....27....8A). 12| A white or yellow star, J-H=0.529 (2MASS). 13| P~62d (NSVS data) is possible. 14| NSVS data show variations with the same period. 15| 1-day aliases of a twice shorter period are strong. 16| P=45d (NSVS data). 17| Variable in ASAS-3 data, not included into the ASAS-3 catalog of 17| variable stars. 18| Not identical to V568 Oph (17:59:44.09, +4:59:55.6, J2000). 19| 1-day aliases (0.399278d and 0.285235d) are also quite possible. 20| The periods 83.8d or 92.5d are possible (NSVS data). 21| A double star. 22| P~63.5d (NSVS data) is possible. 23| P=75d (NSVS data). 24| The period 0.286864d (type EW) is also quite possible. 25| O'Connell effect. 26| A 1-day alias, P=0.49813d, is possible. 27| P~78d (NSVS data) is possible. 28| P~150d (NSVS data) is possible. 29| P~130d (NSVS data) is possible. 30| A twice shorter period and type HADS are possible. 31| P=58d (NSVS data). 32| P=48d (NSVS data). 33| P=62d (NSVS data). 34| P=0.305252d is also possible. 35| P~250d (NSVS data) is possible. 36| P~60d (NSVS data) is possible. 37| P~54d (NSVS data) is possible. 38| P~85d (NSVS data) is possible. 39| A 1-day alias, P=0.397451d, is possible. 40| A twice shorter period and type RRAB are possible. 41| The coordinates are from the USNO-A2.0 catalog. 42| P=81d (NSVS data). 43| Possibly, the minima are deeper. 44| P~82d (NSVS data) is possible. 45| A 1-day alias, P=0.081429d, is possible. ---------------------------------------------------------------------