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Latest Details
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Name
  OGLEII DIA BUL-SC17 V1595  
AAVSO UID
--  
Constellation
Sagittarius Sequence
J2000.0
18 11 33.55 -26 22 07.9  (272.88979 -26.36886) Search nearby
B1950.0 18 08 26.68 -26 22 50.9
Proper motion
RA: 13.2 +/- 6.7 mas/yDec: -14.9 +/- 6.6 mas/ySource: UCAC4
Galactic coord. 5.093 -3.697
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
2MASS J18113355-2622079 ASASSN-V J181133.59-262206.5 OGLE BUL-SC17 V1595
OGLE BUL-SC17 V1601 OGLE BUL-SC17 V1602 OGLE BUL-SC17 V1607
OGLE BUL-SC17 V1608 OGLE BUL-SC17 V1612 OGLE BUL-SC17 V1613
OGLE BUL-SC17 V1614 OGLE BUL-SC17 V1616  
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Variability type
M
Spectral type --
Mag. range
10.5 - 13.2 Ic
Discoverer --
Epoch
15 May 2000 (HJD 2451680): Ephemeris
Outburst --
Period 435: d
Rise/eclipse dur. --
Remarks
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References
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1 N.Matsunaga, H.Fukushi, Y.Nakada, MNRAS 364, 117, 2005. 2005MNRAS.364..117M
2 M.K. Szymanski, 2005, Acta Astron. 55, 43 (online data) 2005AcA....55...43S
3 Groenewegen M.A.T., A+A 443, 143, 2005. 2005A&A...443..143G
External Links
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Location    Go   
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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 = 7.43H = 6.36K = 5.73J - K = 1.70
AllWISE W1 = 5.30W2 = 4.85W3 = 3.27W4 = 2.39W1 - W2 = 0.45W3 - W4 = 0.88
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 18 11 33.55 -26 22 07.9 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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1 Phase plot Otero, Sebastian Alberto 2011-05-03 20:27 UTC Light curve with OGLE I-data.
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
3 Otero, Sebastian Alberto 2012-05-23 18:36 UTC More artifacts caused by this mira added as cross-IDs
2 Otero, Sebastian Alberto 2011-05-03 20:27 UTC Primary record creation. Range, period and epoch from OGLE data.
1 Admin, VSX 2006-06-07 18:13 UTC Preserved original object data.