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Latest Details
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Log in to retrieve additional aliases from SIMBAD. |
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| Name |
ASAS J174140-1615.6 |
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| AAVSO UID |
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| Constellation |
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| J2000.0 |
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| B1950.0 |
17 38 45.75 -16 14 20.1 |
| Galactic coord. |
10.371 +7.381 |
Other names
(Internal only)
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Please note that aliases shown in grey link to obsolete records.
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2MASS J17413888-1615466 |
ASAS 174140-1615.6 |
ASASSN-V J174138.96-161546.8 |
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GSC 06248-00756 |
IRAS 17387-1614 |
NSVS J1741398-161540 |
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OGLE-BLG-LPV-247219 |
OGLE-IV BLG822.27.20 |
WISE J174138.87-161546.4 |
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| Variability type |
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RCB |
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| Spectral type |
-- |
| Mag. range |
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12.8 - <17.4 V |
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| Discoverer |
-- |
| Epoch |
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| Outburst |
-- |
| Period |
-- |
| Rise/eclipse dur. |
-- |
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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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Period changes? No period could be found combining NSVS and ASAS-3 data. J-K= 1.79. ASAS-3 and NSVS magnitudes contaminated by 2MASS J17413972-1615519 (V= 16.0; sep. 13"), 2MASS J17413843-1615340 (V= 14.85; sep. 14") and GSC 06248-00102 (V= 13.13; sep. 22"). NSVS also contaminated by other nearby stars. Range has been corrected. |
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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 |
Iwanek, P.; et al., 2022, The OGLE Collection of Variable Stars: Nearly
66,000 Mira Stars in the Milky Way |
2022ApJS..260...46I |
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2 |
Tisserand, P.; Clayton, G. C.; Bessell, M. S.; et al., 2020, A plethora of
new R Coronae Borealis stars discovered from a dedicated spectroscopic
follow-up survey |
2020A&A...635A..14T |
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3 |
P.R. Wozniak, S.J. Williams, W.T. Vestrand, V. Gupta, AJ 128, 2965, 2004 |
2004AJ....128.2965W |
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G.Pojmanski, Acta Astronomica 52, 397, 2002. |
2002AcA....52..397P |
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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 = 9.23 | H = 8.38 | K = 7.44 | J - K = 1.79 |
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AllWISE
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W1 = 6.04 | W2 = 4.68 | W3 = 3.23 | W4 = 2.62 | W1 - W2 = 1.36 | W3 - W4 = 0.60 |
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Images
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Supporting Documents
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Revision History
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