Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - I. Motivation and modelling-Reference-Cited by-同舟云学术

Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - I. Motivation and modelling

Published:2007-02-11 Issue:1 Volume:375 Page:278-300
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Wall W. F.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/375/1/278/3094642/mnras0375-0278.pdf

Reference101 articles.

1. A New High‐Resolution CO Map of the Inner 2.́5 of M51. I. Streaming Motions and Spiral Structure

2. Filamentary structure in the Orion molecular cloud

3. Infrared dust and millimeter-wave carbon monoxide emission in the Orion region

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1. GAMMA-RAY OBSERVATIONS OF THE ORION MOLECULAR CLOUDS WITH THEFERMILARGE AREA TELESCOPE;The Astrophysical Journal;2012-08-08

2. Rethinking the N(H2)/I(CO) conversion factor;Monthly Notices of the Royal Astronomical Society;2007-08-01

3. Comparison of13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - III. Systematic effects and scientific implications;Monthly Notices of the Royal Astronomical Society;2007-05-11

4. Comparison of13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - II. The simulations: testing the method;Monthly Notices of the Royal Astronomical Society;2007-05-11