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HCN(1-0) Maser Emission by IR Pumping from Unresolved AGN Disk/Torus Toward the Seyfert 2 Nucleus of M51?

S. Matsushita ; V. Trung Dinh ; F. Boone ; M. Krips ; J. Lim ; Sebastien Muller (Institutionen för rymd- och geovetenskap, Onsala rymdobservatorium)
4th ALMA Science Conference on Revolution in Astronomy with ALMA: The Third Year, Tokyo, Japan, 8-11 December Vol. 499 (2015), p. 153-154.
[Konferensbidrag, refereegranskat]

We present similar to 1 '' (similar to 34 pc) resolution observations of HCN(1-0) together with CO J=1-0, 2-1, and 3-2 toward the Seyfert 2 nucleus of M51 using IRAM PdBI and SMA. HCN shows a strong emission at the nucleus only at the systemic velocity, where no obvious CO emission. HCN(1-0)/CO(1-0) > 2 at this region. Based on our radiative transfer calculations, we suggest that this strong HCN emission is affected by the IR pumping and possibly weak HCN masing. This suggests the presence of an edge-on rotating circumnuclear dense molecular gas disk or torus, which remains unresolved at our resolution.

Nyckelord: Astronomy & Astrophysics

Denna post skapades 2016-03-02.
CPL Pubid: 232643


Institutioner (Chalmers)

Institutionen för rymd- och geovetenskap, Onsala rymdobservatorium (2010-2017)


Astronomi, astrofysik och kosmologi

Chalmers infrastruktur

Onsala rymdobservatorium