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A&A 434, L9-L12 (2005)
DOI: 10.1051/0004-6361:200500103
Letter
XMM-Newton observations of two transient millisecond X-ray pulsars in quiescence
S. Campana1, N. Ferrari1, 2, L. Stella3 and G. L. Israel31 INAF - Osservatorio Astronomico di Brera, via Bianchi 46, 23807 Merate (Lc), Italy
e-mail: campana@merate.mi.astro.it
2 Università degli Studi di Milano, via Celoria 16, 20133 Milano, Italy
3 INAF - Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio Catone (Roma), Italy
(Received 28 December 2004 / Accepted 22 March 2005 )
Abstract
We report on XMM-Newton observations of two X-ray transient millisecond
pulsars (XRTMSPs). We detected XTE J0929-314 with an unabsorbed luminosity of
(0.5-10 keV) at a fiducial distance of 10 kpc. The
quiescent spectrum is consistent with a simple power law spectrum. The upper
limit on the flux from a cooling neutron star atmosphere is about
of
the total flux. XTE J1807-294 instead was not detected. We can put
an upper limit on the source quiescent 0.5-10 keV unabsorbed luminosity
at 8 kpc. These observations strenghten the idea
that XRTMSPs have quiescent luminosities significantly lower than classical
neutron star transients.
Key words: accretion, accretion disks -- binaries: close -- stars: individual: XTE J0929-314, XTE J1807-294 -- stars: neutron
SIMBAD Objects
© ESO 2005
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