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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Revnivtsev et al. 2008
- Bibinfo (this paper at ADS)
- Revnivtsev, M., Sazonov, S., Krivonos, R., Ritter, H., Sunyaev, R. 2008,
A&A, 489, 1121-1127.
- Type
- Observational: Analysis of INTEGRAL survey sample.
- Object(s):
- 14 IPs and candidates (V709 Cas,
V2069 Cyg,
NY Lup,
V2400 Oph,
V2487 Oph,
GK Per,
V1223 Sgr,
V1062 Tau,
IGR J15094-6649,
IGR J16167-4957,
IGR J16500-3307,
IGR J17195-4100GK Per,
IGR J17303-0601, and
1RXS J213344.1+510725,)
as wel as V1432 Aql,
IGR J14536-5522, and
SS Cyg.
- Results
- The authors start with the dubious assumption that the distances to 5 IPs
and 1 polar in the sample are securely known (only one of the 6 is in
fact secure) and purport to derive the spatial distribution and the
X-ray luminosity function of hard X-ray emitting CVs.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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