Query= T CEP 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
--------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------
200003 |T     Cep *|210931.78 +682927.2 |M         |  5.2    |  11.3      |            |V |44177.      |     |   388.14           |54   |M5.5e-M8.8e      |00001 00002|           |-0.043 -0.045|2000.0  | |Hip      |          |T     Cep |
--------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------

_______________Cross-identifications:_______________
T     Cep     = BD   +67 1291                 |     
T     Cep     = BS   08113                    |     
T     Cep     = CRL  2721                     |     
T     Cep     = GSC  4460.02400               |     
T     Cep     = HD   202012                   |     
T     Cep     = Hip  104451                   |     
T     Cep     = IRAS 21088+6817               |     
T     Cep     = IRC  +70168                   |     
T     Cep     = SAO  019229                   |     
____________________________________________________

      Reference to a chart or photograph:
00002. AAVSO Variable Star Charts, AAVSO, Cambridge, Massachusetts

Reference to a study of the star:
00001. GCVS compilers.

__________________________________________________________________

Remark: P var. Max = 2414252 + 386.05d*E (JD2406900 - 20490); Max = 2431086 + 394.93d*E (JD2420490 - 32900); Max = 2440262 + 379.22d*E (JD2432900 - 42200); since JD2442200 Max = 2444171 + 392.7d*E. Mean value of the period is given in the Table. SiO maser.

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