Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: The role of ISM pressure and the Molecular Cloud Dissipation Timescale

Details Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: The role of ISM pressure and the Molecular Cloud Dissipation Timescale Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: The role of ISM pressure and the Molecular Cloud Dissipation Timescale

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ans...325..117d&link_type=references

Astronomische Nachrichten, Vol. 325, Supplement 1, Short Contributions Presented at the Annual Scientific Meeting of the Astrono

Astronomy and Astrophysics

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