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The Astrophysical journal, ISSN 0004-637X, 04/2008, Volume 677, Issue 1, pp. 262 - 275
Recent studies have indicated that the HCN-to-CO(J = 1-0) and HCO+-to-HCN(J = 1-0) ratios are significantly different between galaxies with AGN ( active... 
Galaxies: individual (Arp 220, M82, Markarian 231, NGC 1068, NGC 2140 NGC 3627, NGC 4569, NGC 4826, NGC 5194, NGC 6240, NGC 6946, NGC 6951) | Galaxies: active | Galaxies: ISM | Radio lines: galaxies | Physical Sciences | Astronomy & Astrophysics | Science & Technology
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