The X-ray binary GX 339-4/V821 Ara: the distance, inclination, evolutionary status and mass transfer

Abstract

We consider constraints on the distance, inclination and component masses in the X-ray binary GX 339--4 resulting from published works, and then construct detailed evolutionary models for the donor. From both considerations, and assuming the black-hole nature for the compact object (i.e., its mass $>3{\mathrm{M}}_{\odot }$), the possible donor mass is $\approx$0.5--$1.4{\mathrm{M}}_{\odot }$, the inclination is $\approx {40}^{\circ }$--$60^{\circ }$ and the distance is $\approx$8--12\,kpc. The corresponding mass of the compact object is $\approx$4--$11{\mathrm{M}}_{\odot }$. We then confirm a previous estimate that the theoretical conservative mass transfer rate in GX 339--4 is $\lesssim 10^{-9}{\mathrm{M}}_{\odot }$ yr${}^{-1}$. This is $\gtrsim$10 times lower than the average mass accretion rate estimated from the long-term X-ray light curve. We show that this discrepancy can be solved in two ways. One solution invokes irradiation of the donor by X-rays from accretion, which can temporarily enhance the mass transfer rate. We found that absorption of a $\sim$1 per cent of the irradiating luminosity results in the transfer rate equal to the accretion rate. The time scale at which the transfer rate will vary is estimated to be $\sim$10 yr, which appears consistent with the observations. The other solution invokes non-conservative mass transfer. This requires that $\approx$70 per cent of the transferred mass escapes as a strong outflow and carries away the specific angular momentum comparable to that of the donor.

MNRAS, 9 pages, in press

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• The Donor of the Black-Hole X-Ray Binary MAXI J1820+070
• Disk-jet coupling changes as a possible indicator for outbursts from GX 339-4 remaining within the X-ray hard state
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• Back to business: SLX 1746--331 after 13 years of silence
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• Accretion Geometry of Black Hole X-ray Binaries: Insights from X-ray Observations
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