A Multi-Wave length Survey of the ISM in NGC 628

Adler, D.S., Knapen, J., Fanelli, M.N., Westpfahl, D. and Wakker, B.P. (1999) A Multi-Wave length Survey of the ISM in NGC 628. In: In: Galaxy Dynamics, ASP Conference Series vol.182 :. Astronomical Society of the Pacific, pp. 227-228. ISBN 1-58381-007-2
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Is atomic hydrogen a precursor to or byproduct of the star formation process? Recent evidence suggests that a large percentage of the atomic hydrogen in spiral galaxies could be due to photodissociation of molecular gas by UV radiation from hot young stars.
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Additional information Original paper can be found at http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific
Date Deposited 15 May 2025 16:20
Last Modified 30 May 2025 23:09

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