Probing highly obscured, self-absorbed galaxy nuclei with vibrationally excited HCN-Reference-Cited by-同舟云学术

Probing highly obscured, self-absorbed galaxy nuclei with vibrationally excited HCN

Published:2015-11-18 Issue: Volume:584 Page:A42
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Aalto S.,Martín S.,Costagliola F.,González-Alfonso E.,Muller S.,Sakamoto K.,Fuller G. A.,García-Burillo S.,van der Werf P.,Neri R.,Spaans M.,Combes F.,Viti S.,Mühle S.,Armus L.,Evans A.,Sturm E.,Cernicharo J.,Henkel C.,Greve T. R.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201526410/pdf

Reference72 articles.

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

2. Winds of change – a molecular outflow in NGC 1377?

3. High resolution observations of HCN and HCO+J= 3–2 in the disk and outflow of Mrk 231

4. ASSESSING RADIATION PRESSURE AS A FEEDBACK MECHANISM IN STAR-FORMING GALAXIES

5. Heavily reddened quasars atz∼ 2 in the UKIDSS Large Area Survey: a transitional phase in AGN evolution

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