Cygnus X-1 contains a 21-solar mass black hole -- implications for massive star winds

Abstract

The evolution of massive stars is influenced by the mass lost to stellar winds over their lifetimes. These winds limit the masses of the stellar remnants (such as black holes) that the stars ultimately produce. We use radio astrometry to refine the distance to the black hole X-ray binary Cygnus X-1, which we find to be $2.22_{-0.17}^{+0.18}$ kiloparsecs. When combined with previous optical data, this implies a black hole mass of $21.2\pm 2.2$ solar masses, higher than previous measurements. The formation of such a high-mass black hole in a high-metallicity system constrains wind mass loss from massive stars.

Published online in Science on 2021 February 18; Main (3 figures; 1 Table) + Supplementary (11 figures; 3 Tables)

References in corpus (21)

• Modules for Experiments in Stellar Astrophysics (MESA)
• Mass loss from hot massive stars
• The third realization of the International Celestial Reference Frame by very long baseline interferometry
• Distinguishing Spin-Aligned and Isotropic Black Hole Populations With Gravitational Waves
• Bright OB stars in the Galaxy - III. Constraints on the radial stratification of the clumping factor in hot star winds from a combined Halpha, IR and radio analysis
• A 15.65 solar mass black hole in an eclipsing binary in the nearby spiral galaxy Messier 33
• The Masses and Spins of Neutron Stars and Stellar-Mass Black Holes
• A wide star-black-hole binary system from radial-velocity measurements
• On IC 10 X-1, the Most Massive Known Stellar-Mass Black Hole
• Estimating distances from parallaxes. II. Performance of Bayesian distance estimators on a Gaia-like catalogue
• Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star
• The Orbital Period of the Wolf-Rayet Binary IC 10 X-1; Dynamic Evidence that the Compact Object is a Black Hole
• Astrometric accuracy of phase-referenced observations with the VLBA and EVN
• The jet-powered optical nebula of Cygnus X-1
• Not so fast: LB-1 is unlikely to contain a 70 $M_{\odot }$ black hole
• Radio Frequency Timing Analysis of the Compact Jet in the Black Hole X-ray Binary Cygnus X-1
• Wind mass-loss rates of stripped stars inferred from Cygnus X-1
• A 33 hour period for the Wolf-Rayet/black hole X-ray binary candidate NGC 300 X-1
• Techniques for Accurate Parallax Measurements for 6.7-GHz Methanol Masers
• Jet radio emission in Cygnus X-1 and its orbital modulation
• Global Simulations of the Interaction of Microquasar Jets with a Stellar Wind in High-Mass X-ray Binaries

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