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Name
  OGLE BUL-SC35 692678  
AAVSO UID
000-BLH-416 (No observations)  
Constellation
Sagittarius Sequence
J2000.0
18 05 00.35 -27 53 21.9  (271.25146 -27.88942) Search nearby
B1950.0 18 01 51.25 -27 53 35.7
Proper motion
RA: 3.0 +/- 6.8 mas/yDec: -23.6 +/- 6.8 mas/ySource: UCAC4
Galactic coord. 3.054 -3.154
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
2MASS J18050035-2753217 CMC15 J180500.3-275321 GSC2.3 S9TK037974
OGLE BUL-SC36 V4779 UCAC4 311-150288 USNO-B1.0 0621-0797025
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Variability type
M
Spectral type --
Mag. range
15.2: - <17.0 V
Discoverer --
Epoch
05 Oct 1997 (HJD 2450727) Ephemeris
Outburst --
Period 217 d
Rise/eclipse dur. --
Remarks
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1 Otero, Sebastian Alberto J-K= 1.51. 2MASS position. Elements derived from analysis of light contamination from the real variable (too bright for OGLE) on the constant stars OGLE BUL-SC35 681550 and OGLE BUL-SC36 118238. Range from available magnitudes in astrometric catalogues.
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References
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1 Groenewegen M.A.T., A+A 443, 143, 2005. 2005A&A...443..143G
2 Sumi, T.; et al., 2004, The Optical Gravitational Lensing Experiment 2004MNRAS.348.1439S
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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 = 8.35H = 7.34K = 6.84J - K = 1.50
AllWISE W1 = 6.53W2 = 6.28W3 = 5.75W4 = 5.17W1 - W2 = 0.24W3 - W4 = 0.58
Images
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Supporting Documents
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1 Phase plot Otero, Sebastian Alberto 2014-04-04 22:02 UTC Phase plot using data from the CST stars OGLE BUL-SC35 681550 and OGLE BUL-SC36 118238 contaminated by the nearby mira (that is too bright for OGLE).
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Revision History
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1 Otero, Sebastian Alberto 2014-04-04 22:02 UTC Initial submission.