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 The Hipparcos and Tycho Catalogues (European Space Agency, 1997), ESA SP-1200 (CDS Cat. I/239) {1997ESASP1200.....E}
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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