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Latest Details
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Log in to retrieve additional aliases from SIMBAD. |
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| Name |
bet Aur |
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| AAVSO UID |
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| Constellation |
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| J2000.0 |
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| B1950.0 |
05 55 51.57 +44 56 40.8 |
| Proper motion |
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| Galactic coord. |
167.457 +10.409 |
Other names
(Internal only)
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34 Aur |
ADS 4556 |
ADS 4556 A |
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BD+44 1328 |
CCDM J05596+4457A |
GJ 3375 |
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GSC 02924-02742 |
HD 40183 |
HIP 28360 |
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HR 2088 |
IRAS 05558+4456 |
IRC +40148 |
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Menkalinan |
PPM 48617 |
Renson 10720 |
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SAO 40750 |
SBC7 256 |
TIC 440388263 |
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TYC 2924-2742-1 |
WDS J05595+4457Aa,Ab |
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| Variability type |
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EA/DM |
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| Spectral type |
A2IV+A2IV/V |
| Mag. range |
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1.89 - 1.98 V |
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| Discoverer |
-- |
| Epoch |
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| Outburst |
-- |
| Period |
3.9600514 d |
| Rise/eclipse dur. |
6.4% (6.083 h) |
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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 |
Otero, Sebastian Alberto
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Amplitude has been confirmed to be the same (around 0.08 mag.) according to SMEI data so TESS QLP reductions have an issue. |
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2 |
Otero, Sebastian Alberto
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Hipparcos data (Nov. 1989 — Feb. 1993) show an amplitude of 0.08 mag. (Hp). TESS QLP data (Nov. 2019 — Dec. 2022) show an amplitude of only 0.0022 mag. (TESS). Real or artifact? |
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3 |
GCVS Team |
VB A (B 14.1m, 13", 174deg). Min II 1.98. |
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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 |
Huang, C. X.; et al., 2020, Photometry of 10 Million Stars from the First
Two Years of TESS Full Frame Images: Part I |
2020RNAAS...4..204H |
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2 |
Samus, N. N.; Kazarovets, E. V.; Durlevich, O. V.; et al., 2017, General
Catalogue of Variable Stars: Version GCVS 5.1 (November 2019) |
2017ARep...61...80S |
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3 |
Bob Nelson's O-C files, 2016 |
-- |
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4 |
B.Smith, ApJ 108, 504, 1948. |
1948ApJ...108..504S |
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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 = 1.76 | H = 1.76 | K = 1.78 | J - K = -0.02 |
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AllWISE
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W3 = 2.00 | W4 = 1.89 | W3 - W4 = 0.11 |
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Images
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Supporting Documents
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Revision History
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