X1908+075: A Pulsar Orbiting in the Stellar Wind of a Massive Companion

Abstract

We have observed the persistent but optically unidentified X-ray source X1908+075 with the PCA and HEXTE instruments on RXTE. The binary nature of this source was established by Wen, Remillard, & Bradt (2000) who found a 4.4-day orbital period in results from the RXTE ASM. We report the discovery of 605 s pulsations in the X-ray flux. The Doppler delay curve is measured and provides a mass function of 6.1 Msun which is a lower limit to the mass of the binary companion of the neutron star. The degree of attenuation of the low-energy end of the spectrum is found to be a strong function of orbital phase. A simple model of absorption in a stellar wind from the companion star fits the orbital phase dependence reasonably well and limits the orbital inclination angle to the range 38 to 72 degrees. These measured parameters lead to an orbital separation of 60 to 80 lt-s, a mass for the companion star in the range 9-31 Msun, and an upper limit to the size of the companion of ~22 Rsun. From our analysis we also infer a wind mass loss rate from the companion star of >~ 1.3 x 10^-6 Msun/yr and, when the properties of the companion star and the effects of photoionization are considered, likely >~ 4 x 10^-6 Msun/yr. Such a high rate is inconsistent with the allowed masses and radii that we find for a main sequence or modestly evolved star unless the mass loss rate is enhanced in the binary system relative to that of an isolated star. We discuss the possibility that the companion might be a Wolf-Rayet star that could evolve to become a black hole in 10^4 to 10^5 yr. If so, this would be the first identified progenitor of a neutron star--black hole binary.

arXiv comment16 pages, 11 Postscript figures (some different from those in original version), heavily revised second version includes extended stellar wind model analysis, accepted by ApJ

References in corpus (15)

• Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
• An increased estimate of the merger rate of double neutron stars from observations of a highly relativistic system
• Observations of Accreting Pulsars
• Theoretical Black Hole Mass Distributions
• In-flight Performance of the High Energy X-ray Timing Experiment on the Rossi X-ray Timing Explorer
• On the formation and evolution of black-hole binaries
• Galactic distribution of merging neutron stars and black holes - prospects for short GRB progenitors and LIGO/VIRGO
• Complete RXTE Spectral Observations of the Black Hole X-ray Nova XTE J1550-564
• The Orbit of X Per and Its Neutron Star Companion
• Formation of High Mass X-ray Black Hole Binaries
• PSR J1829+2456: a relativistic binary pulsar
• Discovery of a Black-hole Mass - Period Correlation in Soft X-ray Transients and its Implication for Gamma-Ray Burst and Hypernova Mechanisms
• The formation of black hole low-mass X-ray binaries: through case B or case C mass transfer?
• X 1908+075: An X-ray Binary with a 4.4 day Period
• Evolution of Black Holes in the Galaxy

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