V455 And
V515 And
AE Aqr
FO Aqr
V349 Aqr
XY Ari
V405 Aur
V647 Aur
HT Cam
MU Cam
DW Cnc
V709 Cas
V1025 Cen
V1033 Cas
TV Col
TX Col
UU Col
V2069 Cyg
V2306 Cyg
DO Dra
PQ Gem
V418 Gem
DQ Her
V1323 Her
V1460 Her
V1674 Her
EX Hya
NY Lup
V2400 Oph
V2731 Oph
V3037 Oph
V598 Peg
GK Per
AO Psc
HZ Pup
V667 Pup
WX Pyx
V1223 Sgr
V4743 Sgr
CC Scl
V1062 Tau
AX J1740.1
AX J1832.3
AX J1853.3
CTCV J2056
CXO J174954
IGR J04571
IGR J08390
IGR J15094
IGR J16500
IGR J16547
IGR J17014
IGR J17195
IGR J18151
IGR J18173
IGR J18308
IGR J19267
PBC J0927.8
PBC J1841.1
RX J1804
RX J2015
RX J2113
RX J2133
RX J2306
Swift J0717
Swift J1839
Swift J2006
Swift J2138

Full Catalog

Related Systems

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CC Sculptoris = 1RXS J231532.3-304855 = EC 23128-3105

Link to this object in VSX

A finding chart for CC Scl

SkyView image of CC Scl (see important notes)

  • Equatorial: 23h15m31.80s, -30d48m48.6s (Gaia)
  • Galactic: l=17.24, b=-68.75
Finding Chart:
Schwope et al. (2002)
Optical: G=16.8 (Gaia); X-rays: 1.6x10-11 ergs cm-2s-1 (XMM Slew)
IP Credential:
**** (Confirmed LLIP): The spin period is detected in independent X-ray, UV, and optical data, but only during the superoutburst. While further observations are always desirable, the evidence is strong enough to warrant the "confirmed" status.
  • Orbital: 0.058567233 d = 1.4056136 h = 5060.2089 s
    BJD = 2456668.00638(9) + 0.058567233(8)E
    (Kato et al. 2015) for the orbital dip.
  • Spin: 0.004508d = 6.4915 m = 389.49 s
  • Others: 2607 s
203.3 (200.6-206.3) pc (Gaia EDR3; parallax: 4.892+/-0.070 mas)


  1. Ishioka et al. 2001 (optical photometry)
  2. Chen et al. 2001 (optical spectroscopy)
  3. Schwope et al. 2002 (optical identification)
  4. Tappert, Augusteijn & Maza 2004 (optical photometry)
  5. Woudt et al. 2012 (optical spectroscopy & photometry, and X-rays)
  6. Pretorius, Kingge & Schwope 2013 (space density)
  7. Longa-Pena et al. 2015 (optical spectroscopy)
  8. Kato et al. 2015 (optical photometry)
  9. Szkody et al. 2017 (UV photometry and spectroscopy, and optical photometry)
  10. Hameury & Lasota 2017 (disk instability model fo IPs)
  11. Schwope 2018 (space density)

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Please send your comments, suggestions etc. to Koji.Mukai@nasa.gov and/or Koji.Mukai@umbc.edu
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