Abstract
Since the first detection of neutral hydrogen (H i) by Ewen and Purcell in 1951 [4], H i has been a valuable tool for understanding the structure and dynamics of the Milky Way. The first analysis of H i in the Milky Way was also published in 1951 [14] and surveys of the entire Galaxy were immediately undertaken. In the intervening years the atlas of H i in the Milky Way has been continually updated, culminating most recently with the one arcminute resolution International Galactic Plane Survey.
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McClure-Griffiths, N.M. (1997). New Views of Neutral Hydrogen in the Milky Way. In: Pfalzner, S., Kramer, C., Straubmeier, C., Heithausen, A. (eds) The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics, vol 91. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-18902-9_35
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DOI: https://doi.org/10.1007/978-3-642-18902-9_35
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