Fast orbital shrinkage of black hole X-ray binaries driven by circumbinary disks

Abstract

Recently, the black hole X-ray binary (BHXB) Nova Muscae 1991 has been reported to be experiencing an extremely rapid orbital decay. So far, three BHXBs have anomalously high orbital period derivatives, which can not be interpreted by the standard stellar evolution theory. In this work, we investigate whether the resonant interaction between the binary and a surrounding circumbinary (CB) disk could produce the observed orbital period derivatives. Analytical calculations indicate that the observed orbital period derivatives of XTE J1118+480 and A0620-00 can originate from the tidal torque between the binary and a CB disk with a mass of $10^{-9}{\mathrm{M}}_{\odot }$, which is approximately in agreement with the dust disk mass detected in these two sources. However, Nova Muscae 1991 was probably surrounded by a heavy CB disk with a mass of $10^{-7}{\mathrm{M}}_{\odot }$. Based on the CB disk model and the anomalous magnetic braking theory, we simulate the evolution of the three BHXBs with intermediate-mass donor stars by using the MESA code. Our simulated results are approximately consistent with the observed donor star masses, orbital periods, and orbital-period derivatives. However, the calculated effective temperatures of the donor stars are higher than indicated by the observed spectral types of two sources.

arXiv comment6 pages, 5 figures, accepted for publication by ApJL

References in corpus (36)

• Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
• X-ray Properties of Black-Hole Binaries
• Advection-Dominated Accretion: Underfed Black Holes and Neutron Stars
• Common Envelope Evolution: Where we stand and how we can move forward
• On the formation and evolution of black-hole binaries
• Mass Measurements of Stellar and Intermediate Mass Black-Holes
• A Black Hole of > 6 Solar Masses in the X-ray Nova XTE J1118+480
• The evolution of black-hole mass and angular momentum
• Understanding Compact Object Formation and Natal Kicks: II. The case of XTE J1118+480
• Populating the Galaxy with low-mass X-ray binaries
• Circumbinary disks and cataclysmic variable evolution
• The Halo Black-Hole X-ray Transient XTE J1118+480
• Magnetic Braking of Ap/Bp Stars: Application to Compact Black-Hole X-Ray Binaries
• The UV line spectrum of the soft X-ray transient XTE J1118+480: a CNO processed core exposed
• Orbital Period and Outburst Luminosity of Transient Low Mass X-ray Binaries
• Mid-Infrared Emission from Dust around Quiescent Low-Mass X-ray Binaries
• Fast orbital decays of black hole X-ray binaries: XTE J1118+480 and A0620--00
• MMT Observations of the Black Hole Candidate XTE J1118+480 near and in Quiescence
• Donor Stars in Black-Hole X-Ray Binaries
• The Mass of the Black Hole in the X-ray Binary Nova Muscae 1991
• Chemical Abundances of the Secondary Star in the Black Hole X-ray Binary XTE J1118+480
• The fast spiral-in of the companion star to the black hole XTE J1118+480
• Excess mid-IR emission in Cataclysmic Variables
• Doppler tomography of the black hole binary A0620-00 and the origin of chromospheric emission in quiescent X-ray binaries
• On the Formation of Galactic Black Hole Low-Mass X-ray Binaries
• Doppler and modulation tomography of XTE J1118+480 in quiescence
• Evolution of black-hole intermediate-mass X-ray binaries: the influence of a circumbinary disc
• Evolution of intermediate-mass X-ray binaries driven by magnetic braking of Ap/Bp stars: I. ultracompact X-ray binaries
• Chemical Abundances of the Secondary Star in the Black Hole X-Ray Binary V404 Cygni
• Extremely fast orbital decay of the black hole X-ray binary Nova Muscae 1991
• Evolutionary models of short-period soft X-ray transients: comparison with observations
• WISE Detection of the Galactic Low-Mass X-Ray Binaries
• A Dynamical Study of the Black Hole X-ray Binary Nova Muscae 1991
• Formation of Black Hole Low-Mass X-ray Binaries
• Orbital period decay of compact black hole x-ray binaries: the influence of circumbinary disks?
• A Circumbinary Disk Model for the Rapid Orbital Shrinkage in Black Hole Low-Mass X-ray Binaries

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