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Latest Details
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| Name |
V0653 Sco |
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| AAVSO UID |
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| Constellation |
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| J2000.0 |
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| B1950.0 |
17 45 47.48 -39 12 22.0 |
| Proper motion |
| RA: 1.1 +/- 13.6 mas/y | Dec: -0.4 +/- 13.6 mas/y | Source: UCAC4 |
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| Galactic coord. |
351.558 -5.944 |
Other names

(Internal only)
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Please note that aliases shown in grey link to obsolete records.
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2MASS J17491566-3913165 |
ASAS J174916-3913.3 |
ASAS-RCB-7 |
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ASASSN-V J174915.58-391316.7 |
HV 11687 |
IRAS 17457-3912 |
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OGLE-BLG-LPV-251435 |
OGLE-IV BLG602.31.1229 |
WISE J174915.65-391316.5 |
(Not logged in) Add name
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| Variability type |
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RCB |
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| Spectral type |
-- |
| Mag. range |
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12.4 - <16.8: 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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There are currently no remarks on file for this star.
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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 |
Clayton, G. C., 2012, What are the R Coronae Borealis Stars? |
2012JAVSO..40..539C |
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4 |
P. Tisserand, G.C. Clayton, D.L. Welch, B. Pilecki, L. Wyrzykowski, D. Kilkenny, 2012, arXiv:1211.2475 [astro-ph.SR] |
2012arXiv1211.2475T |
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5 |
P. Tisserand, 2011, arXiv:1110.6579v1 [astro-ph.SR] |
2011arXiv1110.6579T |
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6 |
G.Pojmanski, Acta Astronomica 52, 397, 2002. |
2002AcA....52..397P |
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7 |
H.H.Swope, HA 109, N10, 1943. |
1942AnHar.109...41S |
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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 = 12.15 | H = 10.81 | K = 9.35 | J - K = 2.79 |
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AllWISE
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W1 = 6.71 | W2 = 5.57 | W3 = 4.14 | W4 = 3.37 | W1 - W2 = 1.14 | W3 - W4 = 0.77 |
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Images
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Supporting Documents
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Revision History
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