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Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust

J. D. Soler*, S. Molinari, S. C. O. Glover, R. J. Smith, R. S. Klessen, R. A. Benjamin, P. Hennebelle, J. E. G. Peek, H. Beuther, G. Edenhofer, E. Zari, C. Swiggum, C. Zucker

*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

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