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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 4(452), p. 4128-4144

DOI: 10.1093/mnras/stv1408

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

Journal article published in 2015 by M. Mezcua, M. A. Prieto, J. A. Fernández-Ontiveros, K. Tristram ORCID, N. Neumayer, J. K. Kotilainen
This paper is available in a repository.
This paper is available in a repository.

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Abstract

The distribution of warm molecular gas (1000--3000 K), traced by the near-IR H$_2$ 2.12 $μ$m line, has been imaged with a resolution $