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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Parker, Norton & Mukai 2005
- Bibinfo (this paper at ADS)
- Parker, T.L., Norton, A.J., Mukai, K. 2005, A&A 439, 213-226.
- Type
- Observational: X-ray photometry.
- Object(s)
- AE Aqr,
FO Aqr,
V405 Aur,
BG CMi,
V709 Cas,
V1025 Cen,
TV Col,
TX Col,
V2306 Cyg,
YY Dra,
PQ Gem,
V2400 Oph,
AO Psc,
V1223 Sgr,
V1062 Tau,
as well as LS Peg.
- Results
- ASCA and RXTE archival observations reveal 7 out of 16 systems
studied to have an energy-dependent orbital moudlation (i.e.,
widespread but not ubiquitous). In some systems, orbital modulations
come and go indicating changing accretion geometry.
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This file was last modified on
Monday, 15-Aug-2005 10:27:57 EDT
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