The mass function of GX 339-4 from spectroscopic observations of its donor star

Abstract

We obtained 16 VLT/X-shooter observations of GX 339-4 in quiescence in the period May - September 2016 and detected absorption lines from the donor star in its NIR spectrum. This allows us to measure the radial velocity curve and projected rotational velocity of the donor for the first time. We confirm the 1.76 day orbital period and we find that $K_2$ = $219\pm 3$ km s${}^{-1}$, $\gamma =26\pm 2$ km s${}^{-1}$ and $v\sin i=64\pm 8$ km s${}^{-1}$. From these values we compute a mass function $f(M)=1.91\pm 0.08M_{\odot }$, a factor $\sim 3$ lower than previously reported, and a mass ratio $q=0.18\pm 0.05$. We confirm the donor is a K-type star and estimate that it contributes $\sim 45-50\%$ of the light in the $J$- and H-band. We constrain the binary inclination to $37^{\circ }<i<78^{\circ }$ and the black hole mass to $2.3M_{\odot }<M_{\mathrm{BH}}<9.5M_{\odot }$. GX 339-4 may therefore be the first black hole to fall in the 'mass-gap' of $2-5M_{\odot }$.

arXiv comment11 pages, 7 figures, accepted for publication in ApJ

References in corpus (34)

• X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope
• The Nuclear Equation of State and Neutron Star Masses
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• Automated data reduction workflows for astronomy
• The Black Hole Mass Distribution in the Galaxy
• The Mass Distribution of Stellar-Mass Black Holes
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• The Stagger-grid: A Grid of 3D Stellar Atmosphere Models - I. Methods and General Properties
• The "universal" radio/X-ray flux correlation : the case study of the black hole GX 339-4
• Dynamical Evidence for a Black Hole in GX 339-4
• An Improved Dynamical Model for the Microquasar XTE J1550-564
• X-ray Reflection Spectroscopy of the Black Hole GX 339-4: Exploring the Hard State with Unprecedented Sensitivity
• The EXOSAT data on GX 339-4: further evidence for an ``intermediate'' state
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• Near-Infrared Classification Spectroscopy: H-band Spectra of Fundamental MK Standards
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