The warm molecular gas and dust of Seyfert galaxies: two different phases of accretion?-Reference-Cited by-同舟云学术

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

Published:2015-08-11 Issue:4 Volume:452 Page:4128-4144
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Mezcua M.,Prieto M. A.,Fernández-Ontiveros J. A.,Tristram K.,Neumayer N.,Kotilainen J. K.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/452/4/4128/18232404/stv1408.pdf

Reference96 articles.

1. Recent spectral variations in the active nucleus of NGC 1566

2. Modelling the [Fe ii] λ1.644 μm outflow and comparison with H2 and H+ kinematics in the inner 200 pc of NGC 1068

3. EXTRAGALACTIC CS SURVEY

4. The soft X-ray/NLR connection: a single photoionized medium?

5. THE KINEMATICS AND IONIZATION OF NUCLEAR GAS CLOUDS IN CENTAURUS A

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2. BASS. XXXIV. A Catalog of the Nuclear Millimeter-wave Continuum Emission Properties of AGNs Constrained on Scales ≤ 100–200 pc;The Astrophysical Journal Supplement Series;2023-11-01

3. Limited impact of jet-induced feedback in the multi-phase nuclear interstellar medium of 4C12.50;Astronomy & Astrophysics;2023-04-27

4. Compact jets dominate the continuum emission in low-luminosity active galactic nuclei;Astronomy & Astrophysics;2023-01-31

5. Chemical abundances in Seyfert galaxies – IX. Helium abundance estimates;Monthly Notices of the Royal Astronomical Society;2022-06-21

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