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Name
IRAS 17502-3239
AAVSO UID
000-BLH-454 (No observations)
Constellation
Scorpius
Sequence
J2000.0
17 53 34.62 -32 39 49.9 (268.39425 -32.66386)
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B1950.0
17 50 18.09 -32 39 14.7
Galactic coord.
357.676 -3.379
Other names
(Internal only)
Please note that aliases shown in grey link to obsolete records.
2MASS J17533462-3239498
ASAS J175335-3239.9
ASASSN-V J175334.53-323951.4
CMC15 J175334.6-323950
OGLE BUL-SC24 V2822
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Variability type
M
Spectral type
--
Mag. range
13.5 - <18.5: V
Discoverer
--
Epoch
11 Aug 2005 (HJD 2453594)
Ephemeris
Outburst
--
Period
444 d
Rise/eclipse dur.
--
Remarks
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1
Otero, Sebastian Alberto
J-K= 1.74. Crowded area. AAS-3 magnitudes contaminated by several faint stars. Range has been corrected. 2MASS position. Elements derived from combination of ASAS-3 V data with OGLE data of the constant star OGLE BUL-SC24 415506, contaminated by the real variable (too bright for OGLE).
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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
3
Pojmanski, G., 2002, The All Sky Automated Survey
2002AcA....52..397P
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Catalog Data
Information from selected catalogs obtained by cross-matching to 2 arc seconds using the
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2MASS
J = 5.71
H = 4.62
K = 3.98
J - K = 1.74
AllWISE
W1 = 3.50
W2 = 2.69
W3 = 2.08
W4 = 1.27
W1 - W2 = 0.81
W3 - W4 = 0.81
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1
Phase plot
Otero, Sebastian Alberto
2014-04-08 01:51 UTC
Phase plot using ASAS-3 V data and Ic data from the CST star OGLE BUL-SC24 415506 contaminated by the nearby mira (that is too bright for OGLE) and shifted to the V scale.
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Revision History
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1
Otero, Sebastian Alberto
2014-04-08 01:51 UTC
Initial submission.
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