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

The distribution of warm molecular gas (1000–3000 K), traced by the near-IR H2 2.12 μm line, has been imaged with a resolution

Saved in:
Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2015-10, Vol.452 (4), p.4128-4144
Main Authors: Mezcua, M., Prieto, M. A., Fernández-Ontiveros, J. A., Tristram, K., Neumayer, N., Kotilainen, J. K.
Format: Article
Language:English
Subjects:
Accretion
Astronomy
Dust
Filaments
Gases
Heating
Lanes
Molecules
Morphology
Phases
Radio telescopes
Seyfert galaxies
Stars & galaxies
Citations: Items that this one cites
Items that cite this one
Online Access:Request full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:The distribution of warm molecular gas (1000–3000 K), traced by the near-IR H2 2.12 μm line, has been imaged with a resolution
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stv1408