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Name |
eps Aur |
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AAVSO UID |
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Constellation |
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J2000.0 |
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B1950.0 |
04 58 22.53 +43 45 05.4 |
Proper motion |
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Galactic coord. |
162.788 +1.179 |
Other names

(Internal only)
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Variability type |
E-DO/GS+SRD |
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Spectral type |
A8Ia-F2epIa+BV |
Mag. range |
2.92 - 3.83 V |
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Discoverer |
-- |
Epoch |
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Outburst |
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Period |
9892 d (27.08 y) |
Rise/eclipse dur. |
7.6% (107 weeks) |
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Remarks
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Some references may be clicked to view in new window. Roll over index number to view submission details.
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1 |
GCVS Team |
VB A (B 14.0m, 21", 224deg). d = 0.037P. Survey of the physical properties of the system [O.Struve, PASP 68, 27, 1956., K.O.Wright, JRAS Can 49, 221, 1955., H.A.Abt, ApJ 126, 138, 1957., I.M.Kopylov, R.N.Kumajgorodskaya, Izv. Krymsk. Astrofiz. Obs. 29, 251, 1963., M.Hack, Mem SAIt 32, F.4, 1961==Milano-Merate Contr N185, 1962., Kh.Albo, Tartu Publ 45, 284, 1977.]. The spectrum probably varies even outside eclipses. The eclipses are probably due to a disk of gas and dust surrounding the hot companion. The brightness has physical fluctuations with the amplitude up to 0.24m and the cycle about 110d [C.M.Huffer, ApJ 76, 1, 1932.] which hinder revealing the possible Min II. Similar cycle was discovered also in the fluctuations of Vr. |
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References
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Click reference title/citation to view in new window. Roll over index number to view submission details.
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1 |
T. Jayasinghe, K. Z. Stanek, C. Kochanek, et al., 2019 (in preparation) |
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2 |
Zhou, G.; Rappaport, S.; Nelson, L.; et al., 2018, Occultations from an Active Accretion Disk in a 72-day Detached Post-Algol System Detected by K2 |
2018ApJ...854..109Z |
3 |
Kh.Albo, Tartu Publ. 39, 82, 1971. |
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External Links
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Location
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Catalog Data
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Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
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2MASS
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J = 1.88 | H = 1.70 | K = 1.53 | J - K = 0.35 |
AllWISE
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W3 = 1.72 | W4 = 1.38 | W3 - W4 = 0.35 |
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Images
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Supporting Documents
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Campaigns/Programs
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Individual campaigns
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Revision History
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