Synthetic [C ii] emission maps of a simulated molecular cloud in formation-Reference-Cited by-同舟云学术

Synthetic [C ii] emission maps of a simulated molecular cloud in formation

Published:2018-09-18 Issue:4 Volume:481 Page:4277-4299
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Franeck A¹,Walch S¹,Seifried D¹,Clarke S D¹^ORCID,Ossenkopf-Okada V¹,Glover S C O²,Klessen R S²³,Girichidis P⁴,Naab T⁵,Wünsch R⁶,Clark P C⁷,Pellegrini E²,Peters T⁵

Affiliation:

1. I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, D-50937 Köln, Germany

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

3. Universität Heidelberg, Institut für wissenschaftliches Rechnen (IWR), Im Neuenheimer Feld 205, D-69120 Heidelberg, Germany

4. Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany

5. Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, D-85748 Garching, Germany

6. Astronomical Institute, Czech Academy of Sciences, Bocni II 1401, CZ-141 00 Prague, Czech Republic

7. School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA, Wales, UK

Funder

European Research Council

Czech Science Foundation

European Community’s Seventh Framework Programme

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/4/4277/25893294/sty2507.pdf

Reference88 articles.

1. Radiative transfer meets Bayesian statistics: where does a galaxy's [C ii] emission come from?

2. SHOCK-ENHANCED C+EMISSION AND THE DETECTION OF H2O FROM THE STEPHAN'S QUINTET GROUP-WIDE SHOCK USINGHERSCHEL

3. Fine‐Structure Excitation of C+and Si+by Atomic Hydrogen

4. Synthetic observations of molecular clouds in a galactic centre environment – I. Studying maps of column density and integrated intensity

5. Carbon in different phases ([CII], [CI], and CO) in infrared dark clouds: Cloud formation signatures and carbon gas fractions

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