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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Hllier, & Mukai 2004
- Bibinfo (this paper at ADS)
- Hellier, C., Mukai, K. 2004, MNRAS 352, 1037-1040.
- Type
- Observational: X-ray spectroscopy.
- Object(s)
- EX Hya,
GK Per,
AO Psc, and
V1223 Sgr,
as well as AM Her.
- Results
- Chandra HETG observations resolve the Fe Kalpha complex in magnetic
CVs cleanly into H-like, He-like, and fluorescent, and suggest structures
within these components. No Doppler shift is observed, and the lines
are not broad as was claimed from ASCA data. GK Per shows a shoulder
in the 6.4 keV line.
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This file was last modified on
Monday, 02-Aug-2004 11:30:29 EDT
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