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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Cropper et al 1999
- Bibinfo (this paper at ADS)
- Cropper, M., Wu, K., Ramsay, G., Kocabiyik, A. 1999, MNRAS 306, 684-690.
- Type
- Modelling: Post-shock flow with gravity.
- Object(s)
- AE Aqr,
FO Aqr,
XY Ari,
BG CMi,
TV Col,
TX Col,
PQ Gem,
EX Hya,
AO Psc,
and a bunch of polars.
- Results
- A refinement of the shock model including the proper treatment of
the gravitational potential, leading to a lower shock temperature.
Inferred (from X-ray spectra) white dwarf masses are revised.
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This file was last modified on
Saturday, 04-Jan-2003 15:54:05 EST
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