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
|
Scaringi et al. 2010
- Bibinfo (this paper at ADS)
- Scaringi, S., Bird, A.J., Norton, A.J., Knigge, C., Hill, A.B.,
Clark, D.J., Dean, A.J., McBride, V.A., Barlow, E.J., Bassani, L.,
Bazzano, A., Fiocchi, M., Landi, R. 2010, MNRAS, 401, 2207-2218.
- Type
- Observational: Hard X-rays.
- Object(s)
- Confirmed IPs AE Aqr,
FO Aqr,
XY Ari,
V405 Aur,
MU Cam,
BG CMi,
V709 Cas,
TV Col,
TX Col,
V2069 Cyg,
YY Dra,
PQ Gem,
EX Hya,
NY Lup,
V2400 Oph,
GK Per,
AO Psc,
V1223 Sgr,
V1062 Tau,
IGR J00234+6141,
IGR J15094-6649,
IGR J17303-0601,
SWIFT J0732.5-1331, and
1RXS J213344.1+510725;
Candidade IPs TW Pic,
IGR J08390-4833,
IGR J16167-4957,
IGR J16500-3307,
IGR J17195-4100,
V2487 Oph,
IGR J18173-2509,
IGR J18303-1232,
AX J1832.3-0840, and
IGR J19267+1325;
Polars BY Cam, V834 Cen,
IGR J14536-5522, and
V1432 Aql;
as well as SS Cyg and
XSS J12270-4859.
- Results
- IBIS catalog and Swift/BAT and Suzaku/HXD observations are used to
study the population of hard X-ray emitting megnetic CVs.
Correlation between hard X-ray hardness and spin-to-orbital period
ratio is found in the sample.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
|
