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
|
Landi et al. 2009
- Bibinfo (this paper at ADS)
- Landi, R., Bassani, L., Dean, A.J., Bird, A.J., Fiocchi, M., Bazzano, A.,
Nousek, J.A., Osborne, J.P. 2009, MNRAS 392, 630-640.
- Type
- Observational: X-rays.
- Object(s)
- FO Aqr,
MU Cam,
V709 Cas,
V2069 Cyg,
NY Lup,
V2400 Oph,
GK Per,
V1223 Sgr,
IGR J00234+6141,
IGR J15094-6649,
IGR J16167-4957,
IGR J16500-3307,
IGR J17195-4100,
IGR J17303-0601, and
1RXS J213344.1+510725
among IPs and IP candidates; polars BY Cam, V834 Cen,
V1432 Aql, and
IGR J14536-5522;
the dwarf novae SS Cyg; the recurrent nova
V2487 Oph; and the
peculiar system, XSS J12270-4859.
- Results
- INTEGRAL/IBIS spectra of 22 objects (21 CVs and XSS J12270) have been
investigated, resulting in an average Bremsstrahlung temperature of
22 keV (but ranging from 7 keV for MU Cam to 56 keV for V2487 Oph).
For 11 objects, IBIS data are combined with Swift/XRT data, allowing
investigation of the 6.4 keV line, the complex absorber, and the
soft component.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
|
