IPs

V455 And
V515 And
AE Aqr
FO Aqr
V349 Aqr
XY Ari
V405 Aur
V647 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
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
EI UMa
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
LAMOST 0240
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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DW Cancri

Link to this object in VSX

A finding chart for DW Cnc

SkyView image of DW Cnc (see important notes).

Position
  • Equatorial: 07h58m53.01s, +16d16m45.2s (Gaia)
  • Galactic: l=205.34, b=+22.06
Finding Chart:
?
Brigntness:
Optical: G=15.5 (Gaia); X-rays: 1.8x10-11 ergs cm-2s-1 (4XMM-DR11)
IP Credential:
***** (Ironclad LLIP): The orbital, spin and sideband periods all appear well established in the optical, and the spin period has been confirmed in X-rays.
Periods:
  • Orbital: 0.05979267 d = 1.435024 hr = 5166.087 s
    T0 = HJD 2452620.7902(6) + 0.05979267(18) E
    (Emission line velocity; Patterson et al. (2004))
  • Spin: 0.02679429 d = 38.58378 min = 2315.027 s
    T0 = HJD 2452620.7618(3) + 0.02679429(4) E
    (Emission line velocity; maximum blueshift 0.27+/-0.05 cycles before maximum light; Patterson et al. (2004))
  • Others: Beat period (0.04854 d = 69.8956 min = 4193.7358 s) seen in optical photometry.
    Tmin = HJD 2452614.0195(7)+0.0485509(7) E
    (Patterson et al. (2004))
Inclination:
?
Distance:
203.12 (201.39-204.74) pc (Gaia EDR3; parallax: 4.882+/-0.039 mas)

References

  1. Uemura et al. 2002 (optical photometry)
  2. Rodriguez-Gil et al. 2004 (optical spectroscopy & photometry)
  3. Patterson et al. 2004 (optical spectroscopy & photometry)
  4. Thorstensen, Lepine & Shara 2008 (parallax measurement)
  5. Brunschweiger et al. 2009 (X-rays)
  6. Hameury & Lasota 2017 (disk instability model for IPs)
  7. Barrett et al. 2017 (radio)
  8. Nucita et al. 2019 (X-rays)
  9. Segura Montero, Ramirez & Echevarria 2020 (optical spectroscopy)
  10. Simon 2021 (optical photometry)
  11. Duffy et al. 2022 (optical photometry)
  12. Ramirez et al. 2022 (optical photometry and spectroscopy)


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