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
V2069 Cyg
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
SDSS J233325
XSS 00564
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Brunschweiger et al. 2009
- Bibinfo (this paper at ADS)
- Brunschweiger, J., Greiner, J., Ajello, M., Osborne, M., A&A 496,
121-127.
- Type
- Observational: X-rays.
- Object(s)
- FO Aqr,
XY Ari,
V405 Aur,
MU Cam,
V709 Cas,
V1025 Cen,
BG CMi,
TV Col,
TX Col,
V2306 Cyg,
YY Dra,
PQ Gem,
EX Hya,
NY Lup,
V2400 Oph,
GK Per,
AO Psc,
V1223 Sgr,
V1062 Tau,
IGR J00234+6141,
Swift J0732.5-1331,
IGR J17303-0601, and
1RXS J213344.1+510725
as IPs detected with BAT;
AE Aqr,
HT Cam,
DW Cnc,
UU Col,
DQ Her, and
WX Pyx
are undetected.
- Results
- MPE's own analysis of the BAT survey data (for the first 2.5 years
of operation) have detected 22 of the 28 IPs they searched for.
BAT spectra are fitted with Bremsstrahlung and accretion column
models, and the white dwarf masses are derived.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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