Herschel/PACS spectroscopy of NGC 4418 and Arp 220: H2O, H218O, OH,18OH, O I, HCN, and NH3-Reference-Cited by-同舟云学术

Herschel/PACS spectroscopy of NGC 4418 and Arp 220: H2O, H218O, OH,18OH, O I, HCN, and NH3

Published:2012-04-18 Issue: Volume:541 Page:A4
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

González-Alfonso E.,Fischer J.,Graciá-Carpio J.,Sturm E.,Hailey-Dunsheath S.,Lutz D.,Poglitsch A.,Contursi A.,Feuchtgruber H.,Veilleux S.,Spoon H. W. W.,Verma A.,Christopher N.,Davies R.,Sternberg A.,Genzel R.,Tacconi L.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201118029/pdf

Reference121 articles.

1. Luminous HC3N line and the HCN/HCO+ ratio in NGC 4418

2. Overluminous HNC line emission in Arp 220, NGC 4418 and Mrk 231. Global IR pumping or XDRs?

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

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

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