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Table · dataset · 2022

X-ray spectral study of 57 local U/LIRGs

Listed in IVOA Registry (Virtual Observatory)

We perform a systematic X-ray spectroscopic analysis of 57 local luminous and ultraluminous infrared galaxy systems (containing 84 individual galaxies) observed with the Nuclear Spectroscopic Telescope Array and/or Swift/BAT.

Description

Combining soft X-ray data obtained with Chandra, XMM-Newton, Suzaku, and/or Swift/XRT, we identify 40 hard (>10keV) X-ray-detected active galactic nuclei (AGNs) and constrain their torus parameters with the X-ray clumpy torus model XCLUMPY.

Among the AGNs at z<0.03, for which sample biases are minimized, the fraction of Compton-thick (N_H_>=10^24^cm^-2^) AGNs reaches 64_-15_^+14^% (6/9 sources) in late mergers, while it is 24_-10_^+12^% (3/14 sources) in early mergers, consistent with the tendency reported by Ricci+ (2017MNRAS.468.1273R). We find that the bolometric AGN luminosities derived from the infrared data increase but the X-ray to bolometric luminosity ratios decrease with merger stage.

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The X-ray-weak AGNs in late mergers ubiquitously show massive outflows at subparsec to kiloparsec scales. Among them, the most luminous AGNs (L_bol,AGN_~10^46^erg/s) have relatively small column densities of <~10^23^cm^-2^ and almost super-Eddington ratios ({lambda}Edd~1.0). Their torus covering factors (CT^(22)^~0.6) are larger than those of Swift/BAT-selected AGNs with similarly high Eddington ratios.

These results suggest a scenario where, in the final stage of mergers, multiphase strong outflows are produced due to chaotic quasi-spherical inflows, and the AGN becomes extremely X-ray weak and deeply buried due to obscuration by inflowing and/or outflowing material.

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Catalogue records · 2

Topics

Stated by source
Infrared · Optical · Radio · X-Ray
Inferred from text
Astronomical sciences 74% · Computed tomography 50%
Provenance · 1 source records, 13 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/apjs/257/6111 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (74%)
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:infraredsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:radiosource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:x-raysource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].local:modality:ctenrichment · IVOA Registrykeyword-concept-rules@1.0.0title+description (50%)
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
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updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0