Journal article icon

Journal article

The Galaxy Activity, Torus, and Outflow Survey (GATOS)

Abstract:
We use JWST/MIRI MRS spectroscopy of a sample of six local obscured type 1.9/2 active galactic nuclei (AGN) to compare their nuclear mid-IR absorption bands with the level of nuclear obscuration traced by X-rays. This study is the first to use subarcsecond angular resolution data of local obscured AGN to investigate the nuclear mid-IR absorption bands with a wide wavelength coverage (4.9–28.1 μm). All the nuclei show the 9.7 μm silicate band in absorption. We compare the strength of the 9.7 and 18 μm silicate features with torus model predictions. The observed silicate features are generally well explained by clumpy and smooth torus models. We report the detection of the 6 μm dirty water ice band (i.e., a mix of water and other molecules such as CO and CO2) at subarcsecond scales (∼0.26″ at 6 μm; inner ∼50 pc) in a sample of local AGN with different levels of nuclear obscuration in the range log NHX-Ray (cm−2)∼22 − 25. We find good correlation between the 6 μm water ice optical depths and NHX-Ray. This result indicates that the water ice absorption might be a reliable tracer of the nuclear intrinsic obscuration in AGN. The weak water ice absorption in less obscured AGN (log NHX-ray (cm−2)≲23.0 cm−2) might be related to the hotter dust temperature (> TsubH2O ∼ 110 K) expected to be reached in the outer layers of the torus due to their more inhomogeneous medium. Our results suggest it might be necessary to include the molecular content, such as H2O, aliphatic hydrocarbons (CH−), and more complex polycyclic aromatic hydrocarbon (PAH) molecules, in torus models to better constrain key parameters such as the torus covering factor (i.e., nuclear obscuration)
Publication status:
Published
Peer review status:
Peer reviewed

Actions

Access Document

Authors

More by this author
Institution:
University of Oxford
Role:
Author
ORCID:
0000-0002-9627-5281
More by this author
Role:
Author
ORCID:
0000-0001-6794-2519
More by this author
Institution:
University of Oxford
Role:
Author
More by this author
Role:
Author
ORCID:
0000-0002-4005-9619
More by this author
Role:
Author
ORCID:
0000-0002-2125-4670


Publisher:
EDP Sciences
Journal:
Astronomy & Astrophysics More from this journal
Volume:
681
Pages:
L7-L7
Publication date:
2023-12-06
Acceptance date:
2023-12-01
DOI:
EISSN:
1432-0746
ISSN:
0004-6361


Language:
English
Keywords:
Pubs id:
1598385
Local pid:
pubs:1598385
Source identifiers:
W4389398952
Deposit date:
2026-06-05
ARK identifier:
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP