On the Distances to the X-Ray Binaries Cygnus X-3 and GRS 1915+105
In this paper we significantly improve estimates of distance to the X-ray binary systems Cyg X-3 and GRS 1915+105. We report a highly accurate trigonometric parallax measurement for Cyg X-3 using the Very Long Baseline Array at 43 GHz, placing the source at a distance of ${9.67}_{-0.48}^{+0.53}$ kpc...
Main Authors: | M. J. Reid, J. C. A. Miller-Jones |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acfe0c |
Similar Items
-
Inverse MultiView. II. Microarcsecond Trigonometric Parallaxes for Southern Hemisphere 6.7 GHz Methanol Masers G232.62+00.99 and G323.74–00.26
by: L. J. Hyland, et al.
Published: (2023-01-01) -
Metrics of Astrometric Variability in the International Celestial Reference Frame. I. Statistical Analysis and Selection of the Most Variable Sources
by: Phil Cigan, et al.
Published: (2024-01-01) -
Swift J1727.8–1613 Has the Largest Resolved Continuous Jet Ever Seen in an X-Ray Binary
by: Callan M. Wood, et al.
Published: (2024-01-01) -
The Radio Fundamental Catalog. I. Astrometry
by: L. Y. Petrov, et al.
Published: (2025-01-01) -
Single-band VLBI Absolute Astrometry
by: Leonid Petrov
Published: (2023-01-01)