Tracing the formation of molecular clouds via [C ii], [C i], and CO emission-Reference-Cited by-同舟云学术

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Tracing the formation of molecular clouds via [C ii], [C i], and CO emission

Published:2019-04-20 Issue:4 Volume:486 Page:4622-4637
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Clark Paul C¹^ORCID,Glover Simon C O²,Ragan Sarah E¹^ORCID,Duarte-Cabral Ana¹^ORCID

Affiliation:

1. School of Physics and Astronomy, Queen’s Buildings, The Parade, Cardiff University, Cardiff CF24 3AA, UK

2. Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophysik, Albert-Ueberle-Str. 2, D-69120 Heidelberg, Germany

Funder

Science and Technology Facilities Council

Horizon 2020

Deutsche Forschungsgemeinschaft

European Research Council

Seventh Framework Programme

Marie Skłodowska-Curie

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1119/28490511/stz1119.pdf

Reference91 articles.

1. Modeling primordial gas in numerical cosmology

2. Turbulent Flow–driven Molecular Cloud Formation: A Solution to the Post–T Tauri Problem?

3. Molecular Cloud Formation behind Shock Waves

4. The HI/OH/Recombination line survey of the inner Milky Way (THOR)

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