Radiative transfer meets Bayesian statistics: where does a galaxy's [C ii] emission come from?
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/464/3/3315/18517500/stw2580.pdf
Reference103 articles.
1. The H ii Region/PDR Connection: Self‐consistent Calculations of Physical Conditions in Star‐forming Regions
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2. Star Formation Efficiency in Nearby Galaxies Revealed with a New CO-to-H2 Conversion Factor Prescription;The Astrophysical Journal;2024-01-01
3. α-enhanced astrochemistry: the carbon cycle in extreme galactic conditions;Monthly Notices of the Royal Astronomical Society;2023-11-27
4. The Physical Drivers and Observational Tracers of CO-to-H2 Conversion Factor Variations in Nearby Barred Galaxy Centers;The Astrophysical Journal;2023-06-01
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