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Latest Details
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Log in to retrieve additional aliases from SIMBAD. |
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Name |
V0650 Sct |
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AAVSO UID |
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Constellation |
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J2000.0 |
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B1950.0 |
18 44 56.69 -09 54 04.6 |
Galactic coord. |
23.735 -3.650 |
Other names

(Internal only)
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Please note that aliases shown in grey link to obsolete records.
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2MASS J18474181-0950433 |
ASAS J184741-0950.8 |
ASASSN-V J184741.90-095043.4 |
BV 1708 |
IRAS 18449-0954 |
NSV 11344 |
NSVS 16761346 |
OGLE-GD-LPV-021329 |
OGLE-IV DG1022.14.9 |
USNO-A2.0 0750-14635317 |
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Variability type |
M |
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Spectral type |
-- |
Mag. range |
12.7 - <17.5 V |
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Discoverer |
-- |
Epoch |
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Outburst |
-- |
Period |
235 d |
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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Crowded area. ASAS-3 and NSVS magnitudes contaminated by 2MASS J18474167-0950562 (V= 14.6; sep. 13") and 2MASS J18474338-0950361 (V= 15.6; sep. 24"). NSVS magnitudes also contaminated by GSC 05697-01756 (V= 12.2; sep. 43") and 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 |
2 |
E.V. Kazarovets, N.N. Samus, O.V. Durlevich et al., 2019, The 82nd Name-List of Variable Stars. Part II – RA 18h to 20h and Novae |
2019PZ.....39....3K |
3 |
Benko J.M., Csubry Z., 2007, Acta Astronomica 57, 73 |
2007AcA....57...73B |
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Pojmanski, G., 2002, The All Sky Automated Survey |
2002AcA....52..397P |
5 |
W.Strohmeier, R.Knigge, Bamb Ver 10, No.116, 1975. |
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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 = 7.94 | H = 6.99 | K = 6.43 | J - K = 1.50 |
AllWISE
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W1 = 5.89 | W2 = 5.39 | W3 = 4.79 | W4 = 4.29 | W1 - W2 = 0.50 | W3 - W4 = 0.50 |
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Images
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Supporting Documents
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Revision History
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