1 code implementation • 29 Oct 2017 • Y. Zheng, J. E. G. Peek, M. E. Putman, J. K. Werk
Our analyses show that there is likely to be a large amount of gas at $|v_{\rm LSR}|\leq100$ km s$^{-1}$ hidden in the MW's CGM.
Astrophysics of Galaxies
