Query= V2048 OPH GCVS Query forms
  NNo      GCVS          J2000.0            Type      Max        Min I         Min II       Epoch        Year      Period          M-m/D     Spectrum      References  Other desig. p.m.(as/yr)   Epoch     Ident.     New type    GCVS
--------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
592048 |V2048 Oph *|180015.80 +042207.0 |GCAS+UV:  |  4.55   |   4.85     |            |V |            |     |                    |     |B2-B6IV-VneV     |05150 05288|           |+0.002 -0.013|2000.0  | |Hip      |          |V2048 Oph |
--------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------

_______________Cross-identifications:_______________
V2048 Oph     = BD   +04 3570                 |     
V2048 Oph     = BS   06712                    |     
V2048 Oph     = FLM  Oph 066                  |     
V2048 Oph     = GSC  00438.02741              |     
V2048 Oph     = HD   164284                   |     
V2048 Oph     = Hip  088149                   |     
V2048 Oph     = IRAS 17577+0422               |     
V2048 Oph     = MWC  0278                     |     
V2048 Oph     = SAO  123005                   |     
____________________________________________________

      Reference to a chart or photograph:
05288. F.M.Bateson, A.F.Jones, I.Stranson, Charts for Southern Variables, ser. 5, 1968.

Reference to a study of the star:

05150. A.W.J. Cousins, R.Lake, R.H.Stoy, ROB 121, ser.E, 1966 {1966RGOB..121....1C}

__________________________________________________________________

Remark: SB2 [06598]. In the region of the open cluster Cr 359. Along with irregular light variations typical for be stars there are rapid flares with the amplitudes up to 1.8m (lambda eff = 5800 A) [06150]. It is not excluded that the flares occur on a fainter companion of the system.

----The End----