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

D.S. Adler, J. Knapen, M.N. Fanelli, D. Westpfahl, B.P. Wakker

    Research output: Chapter in Book/Report/Conference proceedingConference contribution

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    Abstract

    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.
    Original languageEnglish
    Title of host publicationIn: Galaxy Dynamics, ASP Conference Series vol.182
    PublisherAstronomical Society of the Pacific
    Pages227-228
    ISBN (Print)1-58381-007-2
    Publication statusPublished - 1999

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