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Name
  OGLE SCO_SC6_160224  
AAVSO UID
000-BJV-910 (No observations)  
Constellation
Scorpius Sequence
J2000.0
17 02 41.52 -44 49 54.9  (255.67300 -44.83193) Search nearby
B1950.0 16 59 03.65 -44 45 39.2
Galactic coord. 342.069 -1.898
Other names

(Internal only)
2MASS J17024151-4449549 ASASSN-V J170241.52-444954.9 GDS_J1702415-444954
GSCC2.3.2 S8Q9047048 OGLE II SCO_SC6_160224 OGLE-GD-LPV-016566
OGLE-IV GD1081.02.36077 VSX J170241.5-444954  
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Variability type
M
Spectral type --
Mag. range
13.556 (1.810) Ic
Discoverer --
Epoch
14 Apr 1999 (HJD 2451283.0) Ephemeris
Outburst --
Period 206.3 d
Rise/eclipse dur. --
Remarks
Some references may be clicked to view in new window. Roll over index number to view submission details.
1 Jansen, R I mag OGLE (Szymanski, 2005, Acta Astron., 55, 43 and Udalski, Kubiak and Szymanski, 1997, Acta Astron., 47, 319). 2MASS position. J=10.640. H=9.459. K=8.851 (2MASS at JD 2451403.5059, i.e. 30 days after maximum)
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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 OGLE SCO_SC6_160224 --
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 = 10.64H = 9.46K = 8.85J - K = 1.79
AllWISE W1 = 7.84W2 = 7.60W3 = 7.04W4 = 6.65W1 - W2 = 0.23W3 - W4 = 0.39
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 17 02 41.52 -44 49 54.9 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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2 Light curve OGLE Jansen, R 2010-07-20 23:24 UTC
1 Phase plot OGLE data Jansen, R 2010-07-20 23:24 UTC
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
2 Otero, Sebastian Alberto 2023-02-22 18:10 UTC Period, mean magnitude and amplitude from 2022ApJS..260...46I. Gaia DR3 position.
1 Jansen, R 2010-07-22 08:29 UTC Initial submission.