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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

Related Systems

Candidates

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Sing et al 2004

Bibinfo (this paper at ADS)
Sing, D.K., Howell, S.B., Szkody, P., Cordova, F.A. 2004, PASP 116, 1056-1060.
Type
Observational: UV spectroscopy.
Object(s)
V405 Aur.
Results
FUSE observations detect broad OVI and CIII lines, and narrow OVI lines. The latter probably originates near the white dwarf surface, and its low (2.5+/-0.5 km/s) radial velocity amplitude indicates a low inclination of this system.


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    This file was last modified on Monday, 08-Nov-2004 13:45:37 EST