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Details for Revision 1
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Name
  VSX J180816.5-314103  
AAVSO UID
--  
Constellation
Sagittarius Sequence
J2000.0
18 08 16.52 -31 41 03.3  (272.06883 -31.68425) Search nearby
B1950.0 18 05 01.56 -31 41 32.4
Galactic coord. 0.064 -5.607
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
ASASSN-V J180816.43-314103.3 DENIS J180816.5-314103 IRAS 18050-3141
OGLE BUL-SC06 V3091 OGLE BUL-SC06 V3092 OGLE BUL-SC06 V3093
OGLE BUL-SC06 V3098 OGLE BUL-SC06 V3099 OGLE BUL-SC06 V3103
USNO-B1.0 0583-0655067    
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Variability type
M
Spectral type --
Mag. range
10.0: - <12.4 I
Discoverer --
Epoch
02 May 1997 (HJD 2450571) Ephemeris
Outburst --
Period 323 d
Rise/eclipse dur. --
Remarks
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1 Otero, Sebastian Alberto The object is too bright for OGLE. Results are from contamination on nearby OGLE BUL-SC06 384504. Minimum magnitude from DENIS I-mag. Maximum magnitude is a conservative value for saturated stars in OGLE.
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References
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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 Groenewegen M.A.T., A+A 443, 143, 2005. 2005A&A...443..143G
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Supporting Documents
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1 Phase plot Otero, Sebastian Alberto 2011-06-01 23:33 UTC Light curve with OGLE I-data for the nearby OGLE BUL-SC06 384504 that is contaminated by the actual mira, which is too bright ofr OGLE.
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
2 Otero, Sebastian Alberto 2023-02-27 20:58 UTC Gaia DR3 position.
1 Otero, Sebastian Alberto 2011-06-01 23:33 UTC Initial submission.

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