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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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
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