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Latest Details
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Name
  2MASS J18111163-2630028  
AAVSO UID
000-BMV-827 (No observations)  
Constellation
Sagittarius Sequence
J2000.0
18 11 11.63 -26 30 02.8  (272.79846 -26.50078) Search nearby
B1950.0 18 08 04.77 -26 30 45.2
Proper motion
RA: -43.8 +/- 7.0 mas/yDec: 6.3 +/- 5.2 mas/ySource: UCAC4
Galactic coord. 4.938 -3.688
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
ASASSN-V J181111.69-263002.4 IRAS R18080-2630 OGLE BUL-SC17 V0708
OGLE BUL-SC17 V0709 OGLE BUL-SC17 V0710 OGLE BUL-SC17 V0713
OGLE BUL-SC17 V0719 OGLE BUL-SC17 V0725 OGLE BUL-SC17 V0726
OGLE BUL-SC17 V0728 OGLE BUL-SC17 V0732 OGLE BUL-SC17 V0751
VSX J181111.6-263002    
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Variability type
M:
Spectral type --
Mag. range
9.2 (>1.0:) Ic
Discoverer --
Epoch
20 Jul 1997 (HJD 2450650): Ephemeris
Outburst --
Period 300: d
Rise/eclipse dur. --
Remarks
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1 Otero, Sebastian Alberto J-K 2.27. Maser. Elements from analysis of OGLEII DIA BUL-SC17 394369, contaminated by light from the actual mira, which is too bright for OGLE. Magnitude from DENIS. Variable period or problems with the contaminated data. Time interval between the 1997 and 1998 maxima is 323 d. Possible strong mean magnitude changes.
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References
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1 Groenewegen M.A.T., A+A 443, 143, 2005. 2005A&A...443..143G
2 The Optical Gravitational Lensing Experiment (online data) 2004MNRAS.348.1439S
External Links
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Catalog Data
Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
2MASS J = 4.71H = 3.04K = 2.44J - K = 2.27
AllWISE W3 = 0.73W4 = -0.04W3 - W4 = 0.78
Images
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Supporting Documents
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2 Phase plot Otero, Sebastian Alberto 2011-06-15 20:42 UTC Phase plot with OGLE I-data for a nearby star contaminated by the variable.
1 Light curve Otero, Sebastian Alberto 2011-06-15 20:42 UTC Light curve showing a possible mean magnitude change affecting the data for the contaminated star.
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Revision History
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1 Otero, Sebastian Alberto 2011-06-15 20:44 UTC Initial submission.