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Latest Details
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Name
  V0368 Per  
AAVSO UID
000-BCW-784 (2565 observations)  
Constellation
Perseus Sequence
J2000.0
02 47 32.62 +34 58 27.9  (41.88592 +34.97442) Search nearby
B1950.0 02 44 28.04 +34 45 57.3
Galactic coord. 148.344 -22.104
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
AAVSO 0241+34 CRTS J024732.6+345827 Downes V0368 Per
GALEX J024732.5+345828 GSC2.3 NCMY009446 Gaia21atj
SON 10510 USNO-B1.0 1249-0039672  
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Variability type
UGSU
Spectral type --
Mag. range
15.2 - 21 CR
Discoverer --
Epoch
--
Outburst --
Period --
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 Gaia Alerts, 2021 (online data) --
2 Coppejans, D. L.; et al., 2016, Statistical properties of dwarf novae-type
cataclysmic variables: the outburst catalogue
2016MNRAS.456.4441C
3 I. Miller, 2012, cvnet-outburst 5096 --
4 Light curve from CRTS/CSS (Drake et al. 2009, ApJ, 696, 870) 2009ApJ...696..870D
5 R.A. Downes et al., 2001, PASP 113, 764 (2006 archival version) 2005JAD....11....2D
6 R.A. Downes et al., 2001, PASP 113, 764 2001PASP..113..764D
7 H.Busch, K.Haeussler, VSS 9, H.2, 125, 1979. 1979VeSon...9..125B
8 N.E.Kurochkin, Perem. Zvezdy Supplement 1, N6, 439, 1973. 1973PZP.....1..439K
9 G.A. Richter, 1969, MitVS 5, 88 1969MitVS...5...88R
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.
AllWISE W1 = 16.91W2 = 17.14W1 - W2 = -0.23
Images
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Supporting Documents
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Campaigns/Programs
 Z CamPaign
Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
5 Otero, Sebastian Alberto 2021-04-05 05:14 UTC Gaia EDR3 position.
4 Bernhard, Klaus 2017-02-01 02:05 UTC PPMXL position. CRTS identification from 2016MNRAS.456.4441C.
3 Admin, VSX 2012-12-09 04:30 UTC Update from [cvnet-outburst 5096 ].
2 Wils, Patrick 2009-08-26 02:04 UTC Magnitude range from CRTS light curve. The large amplitude and low outburst frequency makes UGZ type unlikely.
1 Admin, VSX 2005-12-18 01:33 UTC Initial database population.