IPs
AE Aqr
FO Aqr
XY Ari
V405 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1025 Cen
TV Col
TX Col
UU Col
V2306 Cyg
YY Dra
PQ Gem
DQ Her
EX Hya
NY Lup
V2400 Oph
GK Per
AO Psc
WX Pyx
V1223 Sgr
V1062 Tau
RX J2133
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de Martino et al. 2006b
- Bibinfo (this paper at ADS)
- de Martino, D., Matt, G., Mukai, K., Bonnet-Bidaud, J.-M., Burwitz, V.,
Gaensicke, B.T., Haberl, Mouchet, M. 2006, A&A 454, 287-294.
- Type
- Observational: X-ray spectroscopy and photometry.
- Object(s)
- UU Col.
- Results
- X-ray power spectrum is dominated by the 863 s spin signal, but the 3.5 h
orbital and the 935 s beat signals are also seen (disk overflow accretion).
UV and optical modulations are anti-phased. X-ray spectrum can be fitted
with 0.2 keV and 11 keV optically thin emission and a 50 eV blackbody,
whose ratio is consistent with expectations. Magnetic field is too weak
for UU Col to evolve int a polar.
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This file was last modified on
Sunday, 09-Jul-2006 18:14:02 EDT
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