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Latest Details
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Name
  V1031 Per  
AAVSO UID
--  
Constellation
Perseus Sequence
J2000.0
04 22 06.95 +50 17 29.1  (65.52896 +50.29142) Search nearby
B1950.0 04 18 20.48 +50 10 25.5
Proper motion
RA: -11.3 +/- 7.9 mas/yDec: 19.6 +/- 9.9 mas/ySource: UCAC4
Galactic coord. 153.464 +0.343
Other names

(Internal only)
ASASSN-V J042207.02+501729.0 Edinburgh 2-154 GSC 03337-00125
NSVS 4258133 NSVS 4282794  
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Variability type
LB
Spectral type M4
Mag. range
11.05 - 11.35 R1
Discoverer --
Epoch
--
Outburst --
Period --
Rise/eclipse dur. --
Remarks
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1 2012PZP....12....4K Probably can be identified with IRAS 04182+5010. Type SR is not excluded. Faint close companion 2MASS J04220533+5017418.
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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,
2015, IBVS 6151
2015IBVS.6151....1K
2 A.V. Khruslov, 2012, PZP 12, 4 2012PZP....12....4K
3 Catalogue of Stellar Spectral Classifications (Skiff, 2009-2016) 1971PROE....7...73N
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 = 6.59H = 5.33K = 4.82J - K = 1.77
AllWISE W1 = 4.56W2 = 4.41W3 = 4.29W4 = 3.97W1 - W2 = 0.15W3 - W4 = 0.33
APASS-DR9 B = 16.44V = 13.93g' = 15.11r' = 12.75i' = 10.23B - V = 2.50
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 04 22 06.95 +50 17 29.1 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
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Stellar Association Membership
 NGC 1545 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 2017-12-16 03:25 UTC Spectral type from Skiff (VizieR on-line data: B/mk)
2 Admin, VSX 2015-11-20 02:44 UTC Update from [2015IBVS.6151....1K].
1 Admin, VSX 2012-03-24 01:31 UTC Initial upload.