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Name
  XX Cep  
AAVSO UID
000-BCR-750 (11050 observations)  
Constellation
Cepheus Sequence
J2000.0
23 38 20.29 +64 20 02.7  (354.58454 +64.33408) Search nearby
B1950.0 23 36 00.29 +64 03 25.8
Proper motion
RA: 1.788 +/- 0.083 mas/yDec: -8.666 +/- 0.070 mas/ySource: Gaia DR1
Galactic coord. 115.118 +2.577
Other names

(Internal only)
AAVSO 2333+63 AN 245.1928 BD+63 2026
HD 222217 HIP 116648 IOMC 4288000053
SAO 20743    
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Variability type
EA/SD+DSCT
Spectral type A6V+K3IV
Mag. range
9.20 - 10.32 V
Discoverer Gengler et al. (1928)
Epoch
23 Aug 1981 (HJD 2444839.8022) Ephemeris
Outburst --
Period 2.3373266 d
Rise/eclipse dur. 14%  (7.853 h)
Remarks
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1 Billiaert, Bruno DSCT period = 0.03148 d.
2 GCVS Team Min II 9.26. P var. Min I = 2425096.449 + 2.337340d*E (JD2414930 - 30000); Min I = 2441539.4917 + 2.3373059d*E (JD2430000 - 42300) [P.Battistini, A.Bonifazi, A.Guarnieri, IBVS N1325, 1977.]. Since JD2441500 - see Table.
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References
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1 Koo, Jae-Rim; et al., 2016, Time-series spectroscopy of the pulsating
eclipsing binary XX Cephei
2016arXiv160201935K
2 Bob Nelson's O-C files, 2016 --
3 J. Alfonso-Garzon, A. Domingo, J.M. Mas-Hesse, A. Gimenez, 2012,
arXiv:1210.0821 [astro-ph.IM] (online info)
2012arXiv1210.0821A
4 H.Schneller, VBB 8, N6, 1931. --
5 CALEB - Catalog and AtLas of Eclipsing Binaries --
6 General Catalogue of Variable Stars, 4th Edition, Volumes I-III, P.N.
Kholopov et al.
--
External Links
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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 = 8.46H = 8.26K = 8.18J - K = 0.28
AllWISE W1 = 8.18W2 = 8.20W3 = 8.08W4 = 7.82W1 - W2 = -0.01W3 - W4 = 0.27
APASS-DR9 B = 10.40V = 10.13g' = 10.45r' = 10.13i' = 10.07B - V = 0.27
Images
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Supporting Documents
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Revision History
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3 Billiaert, Bruno 2016-02-14 00:09 UTC Variability type, spectral type and discoverer from 2016arXiv160201935K.
2 Admin, VSX 2010-01-05 04:43 UTC Update from the GCVS version of November 2009.
1 Admin, VSX 2005-12-18 01:33 UTC Initial upload.