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Latest Details
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Name
  MACHO 402.47742.51  
AAVSO UID
000-BKQ-884 (No observations)  
Constellation
Sagittarius Sequence
J2000.0
17 55 51.74 -28 48 13.4  (268.96560 -28.80373) Search nearby
B1950.0 17 52 41.30 -28 47 48.4
Galactic coord. 1.262 -1.858
Other names

(Internal only)
2MASS J17555174-2848133 OGLE-BLG-LPV-254657 OGLE-IV BLG505.31.165966
VSX J175551.7-284813    
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Variability type
M
Spectral type --
Mag. range
>13.2 - <17.0 Rc
Discoverer Klaus Bernhard, Stefan Hümmerich
Epoch
14 Apr 1998 (HJD 2450918) Ephemeris
Outburst --
Period 220 d
Rise/eclipse dur. --
Remarks
Some references may be clicked to view in new window. Roll over index number to view submission details.
1 Hümmerich, Stefan Positional data was taken from 2MASS. J-K = 1.706 (2MASS).
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References
Click reference title/citation to view in new window. Roll over index number to view submission details.
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 R.A. Allsman, T.S. Axelrod, 2001, arXiv:astro-ph/0108444 (MACHO online
data)		 2001astro.ph..8444A
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 = 10.11H = 9.00K = 8.40J - K = 1.71
AllWISE W1 = 8.04W2 = 7.70W3 = 7.00W4 = 6.55W1 - W2 = 0.34W3 - W4 = 0.45
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 17 55 51.74 -28 48 13.4 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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1 MACHO 402.47742.51 - lightcurve and phase plot Hümmerich, Stefan 2012-09-18 19:55 UTC MACHO 402.47742.51 - lightcurve and phase plot
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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 22:49 UTC Period from 2022ApJS..260...46I. Gaia DR3 position.
1 Hümmerich, Stefan 2012-09-18 22:30 UTC Initial submission.

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