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<ri:Resource created="2024-10-25T08:58:06Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Mid-IR PAH features of SINGS galaxies</title><shortName>J/ApJ/939/22</shortName><identifier>ivo://CDS.VizieR/J/ApJ/939/22</identifier><altIdentifier>doi:10.26093/cds/vizier.19390022</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang L.</name></creator><creator><name>Ho L.C.</name></creator><creator><name>Li A.</name></creator><date role="Updated">2025-02-12T20:09:27Z</date><date role="Created">2024-10-25T08:58:06Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>interstellar-medium</subject><subject>ultraviolet-photometry</subject><subject>active-galactic-nuclei</subject><subject>star-forming-regions</subject><description>We combined mapping-mode mid-infrared Spitzer spectra with complementary infrared imaging to perform a spatially resolved study of polycyclic aromatic hydrocarbon (PAH) emission from the central regions of 66 nearby galaxies, roughly evenly divided into star-forming systems and low-luminosity active galactic nuclei (AGNs). In conjunction with similar measurements available for quasars, we aim to understand the physical properties of PAHs across a broad range of black hole accretion power, with the goal of identifying observational diagnostics that can be used to probe the effect of AGNs on the host galaxy. Whereas the PAH emission correlates tightly with far-ultraviolet luminosity in star-forming regions, the spatially resolved regions of AGNs tend to be PAH deficient. Moreover, AGN regions exhibit on average smaller PAH 6.2{mu}m/7.7{mu}m and larger PAH 11.3{mu}m/7.7{mu}m band ratios. Although the current data are highly restrictive, they suggest that these anomalous PAH band ratios cannot be explained by the effects of the AGN radiation field alone. Instead, they hint that small grains may be destroyed by the combined effects of radiative processes and shocks, which are plausibly linked to jets and outflows preferentially associated with highly sub-Eddington, radiatively inefficient AGNs. While quasars also present a PAH deficit and unusual PAH band ratios, their characteristics differ in detail compared to those observed in more weakly accreting AGNs, a possible indicator of fundamental differences in their modes of energy feedback.</description><source format="bibcode">2022ApJ...939...22Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/939/22</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : 2MASS All-Sky Extended Source Catalog (XSC) (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/335">II/335 : Revised cat. of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/112/315">J/ApJS/112/315 : Spectroscopic parameters of Seyfert nuclei (Ho+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/633/871">J/ApJ/633/871 : Positions &amp; photometry of HII knots in M51 (Calzetti+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/646/161">J/ApJ/646/161 : Classification of IR galaxies (Dale+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/119/994">J/PASP/119/994 : MIPS 24um calibrators (Engelbracht+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/173/185">J/ApJS/173/185 : GALEX UV atlas of nearby galaxies (Gil de Paz+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/669/959">J/ApJ/669/959 : Warm molecular hydrogen in SINGS galaxies (Roussel+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/658/815">J/ApJ/658/815 : Radio loudness of active galactic nuclei (Sikora+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/656/770">J/ApJ/656/770 : Mid-IR spectrum of star-forming galaxies (Smith+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/693/1821">J/ApJ/693/1821 : The Spitzer infrared nearby galaxies survey (Dale+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/1">J/ApJS/183/1 : Catalog of central stellar velocity dispersions (Ho+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/885">J/ApJ/705/885 : PAH in galaxies at z~0.1 (O'Dowd+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/233">J/ApJS/190/233 : Spectroscopy and abund. of SINGS galaxies (Moustakas+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/719/1191">J/ApJ/719/1191 : Mid-IR indicators of SF and AGN in galaxies (Treyer+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/566/A115">J/A+A/566/A115 : XMM sources in NGC1512/1510 (Ducci+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/790/124">J/ApJ/790/124 : Dust and gas physics of the GOALS sample (Stierwalt+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/470/3071">J/MNRAS/470/3071 : PAH features of AGN (Jensen+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/854/158">J/ApJ/854/158 : z&lt;0.5 PG quasars IR energy distributions (Shangguan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/489/855">J/MNRAS/489/855 : Extended narrow line regions in MaNGA AGN (Chen+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/243/3">J/ApJS/243/3 : Chandra observations of SINGS galaxies (Lehmer+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/884/136">J/ApJ/884/136 : PAH features of star-forming gal. using Spitzer (Xie+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/898/83">J/ApJ/898/83 : BH masses &amp; bulge+disk UV-3.6um colors (Dullo+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/910/124">J/ApJ/910/124 : Star formation rates of low-z QSOs from 1-500um (Xie+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/925/218">J/ApJ/925/218 : Nature of PAH in PG QSOs from Spitzer/IRS sp. 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