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

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

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

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

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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 language	English
Title of host publication	In: Galaxy Dynamics, ASP Conference Series vol.182
Publisher	Astronomical Society of the Pacific
Pages	227-228
ISBN (Print)	1-58381-007-2
Publication status	Published - 1999

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@inproceedings{6aea99b2c4854cde869bedb663ac6d25,

title = "A Multi-Wave length Survey of the ISM in NGC 628",

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.",

author = "D.S. Adler and J. Knapen and M.N. Fanelli and D. Westpfahl and B.P. Wakker",

note = "Original paper can be found at http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific",

year = "1999",

language = "English",

isbn = "1-58381-007-2",

pages = "227--228",

booktitle = "In: Galaxy Dynamics, ASP Conference Series vol.182",

publisher = "Astronomical Society of the Pacific",

address = "United States",

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TY - GEN

T1 - A Multi-Wave length Survey of the ISM in NGC 628

AU - Adler, D.S.

AU - Knapen, J.

AU - Fanelli, M.N.

AU - Westpfahl, D.

AU - Wakker, B.P.

N1 - Original paper can be found at http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific

PY - 1999

Y1 - 1999

N2 - 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.

AB - 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.

M3 - Conference contribution

SN - 1-58381-007-2

SP - 227

EP - 228

BT - In: Galaxy Dynamics, ASP Conference Series vol.182

PB - Astronomical Society of the Pacific

ER -

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

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