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• W2024796675 abstract "The transient X-ray accreting millisecond pulsar XTE J1807-294 was observed during its February/March 2003 outburst by INTEGRAL, partly simultaneously with the XMM-Newton and RXTE satellites. We present here the first study of the 0.5-200 keV broad-band spectra of the source. On February 28, the source spectrum was consistent with thermal Comptonization by electrons of temperature ~40 keV, considerably higher than the value (~10 keV) previously derived from the low energy XMM-Newton data alone. The source is detected by INTEGRAL up to 200 keV with a luminosity in the energy band (0.1-200) keV of erg s-1 (assuming a distance of 8 kpc). 22 days later the luminosity dropped to erg s-1. A re-analysis of XMM-Newton data yields the orbital Doppler variations of the pulse period and refines the previous ephemeris. For this source, with shortest orbital period of any known binary radio or X-ray millisecond pulsar, we constrain the companion mass , assuming minimum mass transfer driven by gravitational radiation. Only evolved dwarfs with a C/O composition are consistent with the Roche lobe and gravitational radiation constraints, while He dwarfs require an unlikely low inclination." @default.
• W2024796675 created "2016-06-24" @default.
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• W2024796675 date "2005-05-30" @default.
• W2024796675 modified "2023-10-18" @default.
• W2024796675 title "INTEGRAL spectroscopy of the accreting millisecond pulsar XTE J1807-294 in outburst" @default.
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• W2024796675 doi "https://doi.org/10.1051/0004-6361:20042575" @default.
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