The warm molecular gas and dust of Seyfert galaxies: two different phases of accretion?

M. Mezcua, M. A. Prieto, J. A. Fernández-Ontiveros +3

The distribution of warm molecular gas (1000--3000 K), traced by the near-IR H${}_2$ 2.12 $\mu$m line, has been imaged with a resolution $<0.5$ arcsec in the central 1 kpc of seven nea…