Molecular line intensities as measures of cloud masses – II. Conversion factors for specific galaxy types
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/378/3/983/18668646/mnras0378-0983.pdf
Reference68 articles.
1. Molecular line intensities as measures of cloud masses - I. Sensitivity of CO emissions to physical parameter variations
2. The abundance gradients across the spiral galaxies NGC 628 and NGC 6946
3. First Detection of Submillimeter [C [CSC]i[/CSC]] Emission in the Small Magellanic Cloud
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