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: UNSPECIFIED.
Copy

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.
Item Type Conference or Workshop Item (Other)
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 19 Aug 2025 01:03

Explore Further

picture_as_pdf
102748.pdf
View Download

Atom BibTeX OpenURL ContextObject in Span OpenURL ContextObject Dublin Core MPEG-21 DIDL Data Cite XML EndNote HTML Citation METS MODS RIOXX2 XML Reference Manager Refer ASCII Citation
Export

Downloads