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Latest Details
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Name
  V2460 Ori  
AAVSO UID
--  
Constellation
Orion Sequence
J2000.0
05 35 27.08 -05 48 52.3  (83.86283 -5.81453) Search nearby
B1950.0 05 33 00.11 -05 50 44.6
Proper motion
RA: 5.9 +/- 4.0 mas/yDec: -3.6 +/- 3.8 mas/ySource: UCAC4
Galactic coord. 209.434 -19.536
Other names

(Internal only)
CSV 100602 GSC 04778-01320 NSV 2333
Parenago 2050 Prag 0262 [CHS2001] 10269
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Variability type
INB
Spectral type --
Mag. range
10.44 - 10.58 J
Discoverer --
Epoch
--
Outburst --
Period --
Rise/eclipse dur. --
Remarks
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1 2011IBVS.5969....1K VB A (B 11.34m, C = V2458 Ori; AB 9", 286deg, AC 6", 349deg, 2001).
2 GCVS Team W-companion (10") is Par 2049 (=GSC 4778.1327).
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References
Click reference title/citation to view in new window. Roll over index number to view submission details.
1 E.V. Kazarovets, N.N. Samus, O.V. Durlevich, N.N. Kireeva, E.N. Pastukhova,
2011, IBVS 5969
2011IBVS.5969....1K
2 Carpenter, J.M., Hillenbrand, L.A., and Skrutskie, M.F. 2001, AJ, 121, No.
6, 3160
2001AJ....121.3160C
3 P.P.Parenago, Trudy GAISh 25, 1954. --
4 L.Gauchet, Zo-Se Ann 18, 1, 1930. --
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 = 10.48H = 9.98K = 9.80J - K = 0.68
AllWISE W1 = 9.22W2 = 8.75W3 = 6.66W4 = 4.71W1 - W2 = 0.47W3 - W4 = 1.95
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 05 35 27.08 -05 48 52.3 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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Stellar Association Membership
 NGC 1976 Open Cluster 2012A&A...548A..97Z
Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
3 Admin, VSX 2011-02-06 17:30 UTC Primary name and details from the 80th GCVS Name-List [2011IBVS.5969....1K].
2 Admin, VSX 2010-01-18 23:18 UTC Position updated to NSV version of June 2009.
1 Admin, VSX 2005-12-18 01:33 UTC Initial upload.