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<ri:Resource created="2018-05-25T10:13:21Z" 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>Herschel FIR spectra of GOALS galaxies</title><shortName>J/ApJ/846/32</shortName><identifier>ivo://CDS.VizieR/J/ApJ/846/32</identifier><altIdentifier>doi:10.26093/cds/vizier.18460032</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Diaz-Santos T.</name></creator><creator><name>Armus L.</name></creator><creator><name>Charmandaris V.</name></creator><creator><name>Lu N.</name></creator><creator><name>Stierwalt S.</name></creator><creator><name>Stacey G.,Malhotra S.</name></creator><creator><name>van der Werf P.P.</name></creator><creator><name>Howell J.H.</name></creator><creator><name>Privon G.C.</name></creator><creator><name>Mazzarella J.M.,Goldsmith P.F.</name></creator><creator><name>Murphy E.J.</name></creator><creator><name>Barcos-Munoz L.</name></creator><creator><name>Linden S.T.</name></creator><creator><name>Inami H.,Larson K.L.</name></creator><creator><name>Evans A.S.</name></creator><creator><name>Appleton P.</name></creator><creator><name>Iwasawa K.</name></creator><creator><name>Lord S.</name></creator><creator><name>Sanders D.B.,Surace J.A.</name></creator><date role="Updated">2021-12-13T06:52:25Z</date><date role="Created">2018-05-25T10:13:21Z</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-sources</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>active-galactic-nuclei</subject><subject>surveys</subject><description>We present an analysis of [OI]_63_, [OIII]_88_, [NII]_122_, and [CII]_158_ far-infrared (FIR) fine-structure line observations obtained with Herschel/PACS, for ~240 local luminous infrared galaxies (LIRGs) in the Great Observatories All-sky LIRG Survey. We find pronounced declines ("deficits") of line-to-FIR continuum emission for [NII]_122_, [OI]_63_, and [CII]_158_ as a function of FIR color and infrared luminosity surface density, {Sigma}_IR_. The median electron density of the ionized gas in LIRGs, based on the [NII]_122_/[NII]_205_ ratio, is n_e_=41cm^-3^. We find that the dispersion in the [CII]_158_ deficit of LIRGs is attributed to a varying fractional contribution of photodissociation regions (PDRs) to the observed [CII]_158_ emission, f([CII]_158_^PDR^)=[CII]_158_^PDR^/[CII]_158_, which increases from ~60% to ~95% in the warmest LIRGs. The [OI]_63_/[CII]_158_^PDR^ ratio is tightly correlated with the PDR gas kinetic temperature in sources where [OI]_63_ is not optically thick or self-absorbed. For each galaxy, we derive the average PDR hydrogen density, n_H_, and intensity of the interstellar radiation field, G, in units of G_0_ and find G/n_H_ ratios of ~0.1-50G_0_.cm^3^, with ULIRGs populating the upper end of the distribution. There is a relation between G/n_H_ and {Sigma}_IR_, showing a critical break at {Sigma}_IR_^*^~5x10^10^L_{sun}_/kpc^2^. Below {Sigma}_IR_^*^, G/n_H_ remains constant, ~0.32G_0_.cm^3^, and variations in {Sigma}_IR_ are driven by the number density of star-forming regions within a galaxy, with no change in their PDR properties. Above {Sigma}_IR_^*^, G/n_H_ increases rapidly with {Sigma}_IR_, signaling a departure from the typical PDR conditions found in normal star-forming galaxies toward more intense/harder radiation fields and compact geometries typical of starbursting sources.</description><source format="bibcode">2017ApJ...846...32D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/846/32</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/VI/139">VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1607">J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/178/280">J/ApJS/178/280 : Compendium of ISO far-IR extragalactic data (Brauher+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/1">J/ApJS/184/1 : Molecular clouds in the LMC by NANTEN. 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MIR AGN fraction from 6.2um PAH equivalent width</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_6.2PAH</name><description>[0.01/0.08]? Uncertainty in 6.2PAH</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S30/S15</name><description>[0/1]? MIR AGN fraction from S_30_/S_15_ ratio diagnostic</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_S30/S15</name><description>[0.01/0.4]? Uncertainty in S30/S15</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_Laurent</name><description>[-] Lower limit flag on Laurent</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Laurent</name><description>[0.1/1]? MIR AGN fraction from Laurent diagram diagnostic</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Laurent</name><description>[0.01/0.2]? Uncertainty in Laurent</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>&lt;AGN&gt;</name><description>[0/1] Average MIR AGN fraction based on all diagnostics</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_&lt;AGN&gt;</name><description>[0/0.4] Uncertainty in &lt;AGN&gt;</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>&lt;AGN&gt;Bol</name><description>[0/1] Average bolometric AGN fraction based on all diagnostics (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_&lt;AGN&gt;Bol</name><description>[0/0.3] Uncertainty in &lt;AGN&gt;Bol</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>