IPs

V455 And
V515 And
AE Aqr
FO Aqr
XY Ari
V405 Aur
V647 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1033 Cas
V1025 Cen
TV Col
TX Col
UU Col
V2069 Cyg
V2306 Cyg
YY Dra
PQ Gem
V418 Gem
DQ Her
V1323 Her
EX Hya
NY Lup
V2400 Oph
V2731 Oph
V598 Peg
GK Per
AO Psc
V667 Pup
WX Pyx
V1223 Sgr
CC Scl
V1062 Tau
EI UMa
AX J1740.1
AX J1740.2
AX J1853.3
IGR J08390
IGR J15094
IGR J16500
IGR J16547
IGR J17195
IGR J18173
IGR J18308
IGR 19267
RX J2133

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Froning et al. 2012

Bibinfo (this paper at ADS)
Froning, C.S., Long, K.S., Gaensicke, B., Szkody, P. 2012, ApJS, 199, A7.
Type
Observational: UV.
Object(s)
AE Aqr, V405 Aur, MU Cam, V709 Cas, TX Col, YY Dra, DQ Her, EX Hya, and NY Lup; also IP candidates LS Peg, and TW Pic; doubtful IP candidate V436 Car and V347 Pup, among FUSE-observed CVs.
Results
The FUSE spectra of CVs are surveyed. Those of IPs are usually usually characterized by strong emission lines and blue continuum emission (from WD photosphere as a whole, hot spots, and/or the disk). YY Dra and probably EX Hya show photosphere-dominated FUV spectra, LS Peg has absorption lines, and V405 Aur looks like high inclination system despite the low inclination values in the literature.


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