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
EI UMa
IGR 00234
IGR 15094
IGR 17303
Swift J0732
RX J0704
RX J1803
RX J2133
XSS 00564
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Mukai et al 2003
- Bibinfo (this paper at ADS)
- Mukai, K., Kinkhabwala, A., Peterson, J.R., Kahn, S.M., Paerels, F.
2003, ApJLett, 586, L77-L80.
- Type
- Observational: X-ray Spectroscopy.
- Object(s)
- EX Hya,
GK Per,
AO Psc, and
V1223 Sgr,
as well as V603 Aql, SS Cyg, and U Gem.
- Results
- Chandra HETG spectra of these 7 CVs can be classified into two types.
EX Hya, with the non-magnetic CVs, have a cooling flow type spectrum.
AO Psc, V1223 Sgr, and GK Per all have hard, power-law like continuum
with weak Fe L lines. The latter group are interpreted with a photoionization
model.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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