no code implementations • 4 Feb 2021 • R. M. Arnason, H. Papei, P. Barmby, A. Bahramian, M. D. Gorski
Comparing positions of Gaia candidate counterparts for XRBs in our sample to positions of spiral arms in the Milky Way, we find that HMXBs exhibit mild preference for being closer to spiral arms; LMXBs exhibit mild preference for being closer to inter-arm regions.
High Energy Astrophysical Phenomena
