The molecular gas in luminous infrared galaxies - I. CO lines, extreme physical conditions and their drivers-Reference-Cited by-同舟云学术

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The molecular gas in luminous infrared galaxies - I. CO lines, extreme physical conditions and their drivers

Published:2012-10-17 Issue:4 Volume:426 Page:2601-2629
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:

Papadopoulos Padelis P.¹,van der Werf Paul P.,Xilouris E. M.²,Isaak K. G.³,Gao Yu⁴,Mühle S.⁵

Affiliation:

1. Max Planck Institute für Radioastronomie; Auf dem Hügel 69; D-53121; Bonn; Germany

2. Institute for Astronomy; Astrophysics; Space Applications & Remote Sensing; National Observatory of Athens; P. Penteli; 15236; Athens; Greece

3. Research and Scientific Support Department; European Space Agency; Keplerlaan 1; 2200; AG Noordwijk; the Netherlands

4. Purple Mountain Observatory; Chinese Academy of Sciences; Nanjing; Jiangsu; 210008; China

5. Argelander-Institut für Astronomie; Auf dem Hügel 71; D-53121; Bonn; Germany

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/426/4/2601/3288480/426-4-2601.pdf

Reference146 articles.

1. Variation of Molecular Line Ratios and Cloud Properties in the Arp 299 Galaxy Merger

2. Detection of HCN, HCO+, and HNC in the Mrk 231 molecular outflow

3. Dust and CO emission towards the centers of normal galaxies, starburst galaxies and active galactic nuclei

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