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Name
  BD+56 2647  
AAVSO UID
000-BLG-022 (72 observations)  
Constellation
Cepheus Sequence
J2000.0
21 47 51.13 +57 11 20.1  (326.96304 +57.18892) Search nearby
B1950.0 21 46 14.00 +56 57 22.0
Proper motion
RA: -6.987 +/- 1.137 mas/yDec: -4.346 +/- 0.673 mas/ySource: Gaia DR1
Galactic coord. 100.005 +2.729
Other names

(Internal only)
2MASS J21475113+5711201 ASASSN-V J214751.00+571119.4 GSC 03976-01677
TYC 3976-1677-1 UCAC4 736-080234  
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Variability type
DSCT
Spectral type --
Mag. range
10.57 - 10.61 Rc
Discoverer Giuseppe Marino
Epoch
06 Dec 2013 (HJD 2456633.2971) Ephemeris
Outburst --
Period 0.16728 d  (4.015 h)
Rise/eclipse dur. --
Remarks
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1 Marino, Giuseppe The observations were performed with the support of Gruppo Astrofili Catanesi at the private observatory of Giuseppe Giardina.
2 Marino, Giuseppe Light curves and their amplitude are given for both the variable star (BD+56 2647) and its optical companion (2MASS J21475113+5711201) not well resolved on the original images.
3 Marino, Giuseppe The amplitude of variation changed from 0.04 mag. (6 Dec. 2013) to 0.01 mag. (17 Dec. 2013). The variable has an optical companion (2MASS J21475157+5711227, V= 13.7:; sep. 4.3") not well resolved on the CCD exposures. However, the stability of this companion was accurately checked by properly positioning the photometric apertures. Claudia Russo, Dosithea Aiello, Xiomara Arena, Caterina Burgio, Brendon Dzema, Ilenia Privitera and Enrica Torrisi (Liceo Linguistico S. Orsola - Catania - ITALY) co-workers.
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References
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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 = 9.35H = 9.11K = 9.03J - K = 0.32
AllWISE W1 = 8.83W2 = 8.84W3 = 8.85W4 = 8.38W1 - W2 = -0.01W3 - W4 = 0.47
APASS-DR9 B = 11.53V = 10.79g' = 11.17r' = 10.63i' = 10.31B - V = 0.74
Images
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Supporting Documents
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2 Light curves for each night Marino, Giuseppe 2013-12-19 23:46 UTC Differential photometry obtained using 1 comparison star very near the variable (2MASS J21475189+5711375). A check star was also used. R_c magnitudes at the max. and min. were determined via ensemble photometry using 3 comparison stars. The R_c magnitude of the comparison stars were deduced from APASS by mean the formulae given by Munari, JAAVSO, 40, 582 (2012).
1 Phase light curve Marino, Giuseppe 2013-12-19 23:46 UTC Phased light curve.
Ephemeris:
HJD(Max) = 2456633.297095 + 0.167280d E
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Revision History
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1 Marino, Giuseppe 2013-12-20 01:33 UTC Initial submission.