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Latest Details
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Name |
V3874 Sgr |
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AAVSO UID |
000-BFJ-205 (No observations) |
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Constellation |
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J2000.0 |
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B1950.0 |
18 26 00.59 -28 25 59.5 |
Proper motion |
RA: -9.6 +/- 4.1 mas/y | Dec: -6.7 +/- 3.5 mas/y | Source: UCAC4 |
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Galactic coord. |
5.101 -8.102 |
Other names

(Internal only)
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Please note that aliases shown in grey link to obsolete records.
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2MASS J18291018-2823595 |
AN 911.1936 |
ASAS J182910-2824.0 |
ASASSN-V J182910.09-282359.7 |
HV 9443 |
OGLE-BLG-LPV-264269 |
OGLE-IV BLG691.06.49253 |
UCAC4 309-220453 |
[MM63] 7-62 |
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Variability type |
M |
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Spectral type |
M6.5: |
Mag. range |
12.5 - <14.8 V |
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Discoverer |
-- |
Epoch |
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Outburst |
-- |
Period |
116.13 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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ASAS-3 magnitudes contaminated by 2MASS J18291033-2824103 (V= 14.9; sep. 11") and 2MASS J18291056-2824141 (V= 15.8; sep. 15"). Range has been corrected. |
2 |
GCVS Team |
P var. Max = 2436035 + 115.3d*E (JD2426000 - 38000); since JD2438000 - see Table. |
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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 |
G.Pojmanski, Acta Astronomica 52, 397, 2002. |
2002AcA....52..397P |
3 |
D.Hoffleit, IBVS N729, 1972. |
1972IBVS..729....1H |
4 |
S.W. McCuskey, R. Mehlhorn, 1963, AJ 68, 319 |
1963AJ.....68..319M |
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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 = 9.33 | H = 8.46 | K = 8.29 | J - K = 1.04 |
AllWISE
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W1 = 8.20 | W2 = 8.05 | W3 = 7.61 | W4 = 7.41 | W1 - W2 = 0.15 | W3 - W4 = 0.20 |
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Images
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Please review Digitized Sky Survey Acknowledgment and Copyright.
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Supporting Documents
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There are currently no supporting documents on file for this star.
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Revision History
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