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
|
Ramsay 2000
- Bibinfo (this paper at ADS)
- Ramsay, G. 2000, MNRAS, 314, 403-408.
- Type
- Observational: Mass determination from X-ray spectroscopy.
- Object(s)
- FO Aqr,
XY Ari,
V405aur,
V709 Cas,
BG CMi,
V1025 Cen,
TV Col,
TX Col,
EX Hya,
V2400 Oph,
AO Psc,
V1223 Sgr, and
V1062 Tau.
- Results
- White dwarf mass determination using RXTE spectra.
IPs appear to have more massive white dwarfs than the isolated
sample.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
|
