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Latest Details
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Name
  V1709 Ori  
AAVSO UID
000-BFQ-289 (1 observation)  
Constellation
Orion Sequence
J2000.0
05 34 52.24 -04 28 16.2  (83.71767 -4.47116) Search nearby
B1950.0 05 32 23.70 -04 30 11.6
Proper motion
RA: 6.3 +/- 3.5 mas/yDec: 7.6 +/- 4.0 mas/ySource: UCAC4
Galactic coord. 208.096 -19.056
Other names

(Internal only)
ASASSN-V J053452.22-042816.2 ASASSN-V J053452.23-042815.9 CSS_J053452.2-042815
Rebull 1532 UCAC4 428-010504  
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Variability type
TTS/ROT
Spectral type --
Mag. range
13.13 (0.18) Ic
Discoverer --
Epoch
--
Outburst --
Period 5.1042203 d
Rise/eclipse dur. --
Remarks
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References
Click reference title/citation to view in new window. Roll over index number to view submission details.
1 Drake, A. J.; et al., 2014, The Catalina Surveys Periodic Variable Star
Catalog (version May 24, 2017)		 2014ApJS..213....9D
2 Rebull, L.M. 2001, AJ, 121, No. 3, 1676. 2001AJ....121.1676R
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 = 12.33H = 11.57K = 11.42J - K = 0.91
AllWISE W1 = 11.31W2 = 11.27W3 = 9.81W4 = 8.19W1 - W2 = 0.04W3 - W4 = 1.61
APASS-DR9 B = 17.00V = 15.56g' = 16.26r' = 14.97i' = 14.22B - V = 1.44
SDSS-DR12 u = 18.57g = 16.18r = 14.85i = 14.11z = 13.64u - g = 2.39r - i = 0.73
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 05 34 52.24 -04 28 16.2 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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Stellar Association Membership
 NGC 1981 Open Cluster 2012A&A...548A..97Z
Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
3 Otero, Sebastian Alberto 2018-08-28 01:44 UTC Type from CSS data. Period from 2014ApJS..213....9D (2017 version). UCAC4 position.
2 Admin, VSX 2010-01-05 04:43 UTC Position updated from the GCVS version of November 2009.
1 Admin, VSX 2006-08-20 03:12 UTC Initial upload.

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