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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Yuasa et al. 2010
- Bibinfo (this paper at ADS)
- Yuasa, T., Nakazawa, K., Makishima, K., Saitou, K., Ishida, M.,
Ebisawa, K., Mori, H., Yamada, H. 2010, A&A, 520, A25.
- Type
- Observational: X-ray Spectroscopy.
- Object(s)
- FO Aqr,
XY Ari,
MU Cam,
BG CMi,
V709 Cas,
TV Col,
TX Col,
YY Dra,
PQ Gem,
EX Hya,
NY Lup,
V2400 Oph,
AO Psc,
V1223 Sgr,
IGR J17303-0601,
IGR J17195-4100, and
1RXS J213344.1+510725.
- Results
- 3-50 keV X-ray spectra of 17 IPs observed with Suzaku are analyzed
to infer the white dwarf mass. In several cases, the current results
disagree with previous studies.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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