Query= eps Aur 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
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089005 |eps   Aur *|050158.13 +434923.9 |EA        |  2.92   |   3.88     |            |V |45513.      |     |  9884.             |08   |A8Iab:           |00001 HIP  |           |+0.000 -0.002|2000.0  | |Hip      |EA        |eps   Aur |
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_______________Cross-identifications:_______________
eps   Aur     = ADS  03605                    |A    
eps   Aur     = BAY  Aur eps                  |     
eps   Aur     = BD   +43 1166                 |     
eps   Aur     = BS   01605                    |     
eps   Aur     = CRL  0670S                    |     
eps   Aur     = FLM  Aur 007                  |     
eps   Aur     = GSC  2907.01275               |     
eps   Aur     = HD   031964                   |     
eps   Aur     = Hip  023416                   |     
eps   Aur     = IRAS 04583+4345               |     
eps   Aur     = IRC  +40109                   |     
eps   Aur     = SAO  039955                   |     
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      Reference to a chart or photograph:

HIP European Space Agency, 1997, The Hipparcos and Tycho Catalogues, ESA SP-1200 {1997HIP...C......0E}

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

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Remark: d = 0.04 P. VB A (B 14.0m, 30", 225deg, 2008; C 11.3m, 43", 276deg, 2008; D 12.0m, 45", 316deg, 2008). Probably eclipses are caused by a gas and dust disk. Besides eclipses, quasi-periodic brightness variations with an amplitude of several tenths of a magnitude and a cycle of 105 - 120 days (e.g., [N0204]). More rapid variations were also reported.

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