CON-quest: Searching for the most obscured galaxy nuclei
Artikel i vetenskaplig tidskrift, 2021

Context. Some luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) host extremely compact (r < 100 pc) and dusty nuclei. The high extinction associated with large column densities of gas and dust toward these objects render them hard to detect at many wavelengths. The intense infrared radiation arising from warm dust in these sources can provide a significant fraction of the bolometric luminosity of the galaxy and is prone to excite vibrational levels of molecules such as HCN. This results in emission from the rotational transitions of vibrationally excited HCN (HCN-vib); the brightest emission is found in compact obscured nuclei (CONs; ςHCN-vib > 1 L⊙ pc-2 in the J = 3-2 transition). However, there have been no systematic searches for CONs, and it is unknown how common they are. Aims. We aim to establish how common CONs are in the local Universe (z < 0.08), and whether their prevalence depends on the luminosity or other properties of the host galaxy. Methods. We conducted an Atacama Large Millimeter/submillimeter Array survey of the rotational J = 3-2 transition of HCN-vib in a volume-limited sample of 46 far-infrared luminous galaxies. Results. Compact obscured nuclei are identified in 38-13+18% of the ULIRGs, 21-6+12% of the LIRGs, and 0-0+9% of the lower luminosity galaxies. We find no dependence on the inclination of the host galaxy, but strong evidence of lower IRAS 25 μm to 60 μm flux density ratios (f25/f60) in CONs (with the exception of one galaxy, NGC 4418) compared to the rest of the sample. Furthermore, we find that CONs have stronger silicate features (s9.7 μm), but similar polycyclic aromatic hydrocarbon equivalent widths (EQW6.2 μm) compared to other galaxies. Along with signatures of molecular inflows seen in the far-infrared in most CONs, submillimeter observations also reveal compact, often collimated, outflows. Conclusions. In the local Universe, CONs are primarily found in (U)LIRGs, in which they are remarkably common. As such systems are often highly disturbed, inclinations are difficult to estimate, and high-resolution continuum observations of the individual nuclei are required to determine if the CON phenomenon is related to the inclinations of the nuclear disks. Further studies of the in- A nd outflow properties of CONs should also be conducted to investigate how these are connected to each other and to the CON phenomenon. The lower f25/f60 ratios in CONs as well as the results for the mid-infrared diagnostics investigated (EQW6.2 μm and s9.7 μm) are consistent with the notion that large dust columns gradually shift the radiation from the hot nucleus to longer wavelengths, making the mid- A nd far-infrared "photospheres"significantly cooler than the interior regions. Finally, to assess the importance of CONs in the context of galaxy evolution, it is necessary to extend this study to higher redshifts where (U)LIRGs are more common.

ISM: Jets and outflows

ISM: Molecules

Galaxies: ISM

Galaxies: Evolution

Galaxies: Nuclei

Författare

Niklas Falstad

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

Susanne Aalto

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Sabine König

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium, Observationssupport

Kyoko Onishi

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

Sebastien Muller

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium, Observationssupport

Mark Gorski

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

Mamiko Sato

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

Flora Stanley

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

F. Combes

Observatoire de Paris

E. Gonzalez-Alfonso

Universidad de Alcala

J. G. Mangum

National Radio Astronomy Observatory

A. S. Evans

University of Virginia

National Radio Astronomy Observatory

Loreto Barcos-Munoz

National Radio Astronomy Observatory

G. Privon

National Radio Astronomy Observatory

S. T. Linden

University of Virginia

T. Diaz-Santos

Idryma Technologias kai Erevnas (FORTH)

Chinese Academy of Sciences

Universidad Diego Portales

S. Martín

Atacama Large Millimeter-submillimeter Array (ALMA)

European Southern Observatory Santiago

K. Sakamoto

Academia Sinica

N. Harada

National Astronomical Observatory of Japan

Academia Sinica

G. A. Fuller

University of Manchester

Instituto de Astrofisica de Andalucía (IAA)

J. S. Gallagher

University of Wisconsin Madison

P. van der Werf

Universiteit Leiden

Serena Viti

University College London (UCL)

Universiteit Leiden

T. R. Greve

University College London (UCL)

Danmarks Tekniske Universitet (DTU)

S. G. Burillo

Observatorio Astronómico Nacional (OAN)

C. Henkel

Max-Planck-Gesellschaft

King Abdulaziz University

M. Imanishi

National Astronomical Observatory of Japan

T. Izumi

National Astronomical Observatory of Japan

Y. Nishimura

National Astronomical Observatory of Japan

University of Tokyo

C. Ricci

Beijing University of Technology

George Mason University

Universidad Diego Portales

S. Muhle

Universität Bonn

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 649 A105

Onsala rymdobservatorium infrastruktur

Vetenskapsrådet (VR) (2017-00648), 2018-01-01 -- 2021-12-31.

Ämneskategorier

Astronomi, astrofysik och kosmologi

Atom- och molekylfysik och optik

Annan fysik

DOI

10.1051/0004-6361/202039291

Mer information

Senast uppdaterat

2021-06-22