Characterizing the Multiphase Origin of [C ii] Emission in M101 and NGC 6946 with Velocity-resolved Spectroscopy-Reference-Cited by-同舟云学术

Characterizing the Multiphase Origin of [C ii] Emission in M101 and NGC 6946 with Velocity-resolved Spectroscopy

Published:2021-07-01 Issue:2 Volume:915 Page:92
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Tarantino Elizabeth^ORCID,Bolatto Alberto D.^ORCID,Herrera-Camus Rodrigo^ORCID,Harris Andrew I.^ORCID,Wolfire Mark^ORCID,Buchbender Christof^ORCID,Croxall Kevin V.^ORCID,Dale Daniel A.^ORCID,Groves Brent^ORCID,Levy Rebecca C.^ORCID,Riquelme Denise^ORCID,Smith J.-D T.^ORCID,Stutzki Jürgen^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abfcc6/pdf

Reference110 articles.

1. Deriving a multivariate αCO conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations

2. A Robust Tip of the Red Giant Branch Distance to the Fireworks Galaxy (NGC 6946)

3. Common-Resolution Convolution Kernels for Space- and Ground-Based Telescopes

4. Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: The KINGFISH Sample

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