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A Parallax Distance to the Microquasar GRS 1915 105 and a Revised Estimate of its Black Hole Mass

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Abstract

  • Using the Very Long Baseline Array, we have measured a trigonometric parallax for the microquasar GRS 1915 105, which contains a black hole and a K-giant companion. This yields a direct distance estimate of 8.6 2.0{-1.6} kpc and a revised estimate for the mass of the black hole of 12.4 2.0-1.8 M . GRS 1915 105 is at about the same distance as some H

Publication Date

  • 2014

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