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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Butters et al. 2007
- Bibinfo (this paper at ADS)
- Butters, O.W., Barlow, E.J., Norton, A.J., Mukai, K. 2007, A&A,
475, L29-L32.
- Type
- Observational: X-ray Photometry and Spectrscopy.
- Object(s)
- Swift J0732.5-1331.
- Results
- The spin period of 512.4 s is clearly established using a 36 ksec
RXTE observation of Swift J0732.5-1331, and it has an X-ray spectrum
typical of IPs, thus confirming its IP status. X-ray orbital modulation
is not seen if the 5.6 hr period seen in optical spectroscopy is correct,
although there appears to be a modulation at the 11.2 hr period suggested
earlier.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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