XMM-Newton spectral and timing analysis of the faint millisecond pulsars PSR J0751+1807 and PSR J1012+5307
Kramer, M.;
Webb, N. A.;
Barret, D.;
Olive, J. -F.;
Cognard, I.;
Löhmer, O.
France, United Kingdom, Germany
Abstract
We present XMM-Newton MOS imaging and PN timing data of the faint millisecond pulsars PSR J0751+1807 and PSR J1012+5307. We find 46 sources in the MOS field of view of PSR J0751+1807 searching down to an unabsorbed flux limit of 3 × 10-15 ergs cm-2 s-1 (0.2-10.0 keV). We present, for the first time, the X-ray spectra of these two faint millisecond pulsars. We find that a power law model best fits the spectrum of PSR J0751+1807, Γ=1.59 ±0.20, with an unabsorbed flux of 4.4× 10-14 ergs cm-2 s-1 (0.2-10.0 keV). A power law is also a good description of the spectrum of PSR J1012+5307, Γ=1.78±0.36, with an unabsorbed flux of 1.2× 10-13 ergs cm-2 s-1 (0.2-10.0 keV). However, a blackbody model cannot be excluded as the best fit to this data. We present some evidence to suggest that both of these millisecond pulsars show pulsations in this X-ray band. We find some evidence for a single broad X-ray pulse for PSR J0751+1807 and we discuss the possibility that there are two pulses per spin period for PSR J1012+5307.
2004
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Astronomy and Astrophysics
XMM-Newton
30
