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<ri:Resource created="2023-01-18T11:50:43Z" 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>SOFIA CII and NII obs. of M101 and NGC6946</title><shortName>J/ApJ/915/92</shortName><identifier>ivo://CDS.VizieR/J/ApJ/915/92</identifier><altIdentifier>doi:10.26093/cds/vizier.19150092</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tarantino E.</name></creator><creator><name>Bolatto A.D.</name></creator><creator><name>Herrera-Camus R.</name></creator><creator><name>Harris A.I.</name></creator><creator><name>Wolfire M.,Buchbender C.</name></creator><creator><name>Croxall K.V.</name></creator><creator><name>Dale D.A.</name></creator><creator><name>Groves B.</name></creator><creator><name>Levy R.C.</name></creator><creator><name>Riquelme D.,Smith J.-DT.</name></creator><creator><name>Stutzki J.</name></creator><date role="Updated">2023-01-19T08:58:58Z</date><date role="Created">2023-01-18T11:50:43Z</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>interstellar-medium</subject><subject>molecular-physics</subject><subject>chemical-abundances</subject><description>The [CII] fine-structure transition at 158{mu}m is frequently the brightest far-infrared line in galaxies. Due to its low ionization potential, C+ can trace the ionized, atomic, and molecular phases of the ISM. We present velocity-resolved [CII] and [NII] pointed observations from SOFIA/GREAT on ~500pc scales in the nearby galaxies M101 and NGC 6946 and investigate the multiphase origin of [CII] emission over a range of environments. We show that ionized gas makes a negligible contribution to the [CII] emission in these positions using [NII] observations. We spectrally decompose the [CII] emission into components associated with the molecular and atomic phases using existing CO (2-1) and HI data and show that a peak signal-to-noise ratio of 10-15 is necessary for a reliable decomposition. In general, we find that in our pointings &gt;~50% of the [CII] emission arises from the atomic phase, with no strong dependence on star formation rate, metallicity, or galactocentric radius. We do find a difference between pointings in these two galaxies, where locations in NGC 6946 tend to have larger fractions of [CII] emission associated with the molecular phase than in M101. We also find a weak but consistent trend for fainter [CII] emission to exhibit a larger contribution from the atomic medium. We compute the thermal pressure of the cold neutral medium through the [CII] cooling function and find log(P_th_/k)=3.8-4.6[K/cm^3^], a value slightly higher than similar determinations, likely because our observations are biased toward star-forming regions.</description><source format="bibcode">2021ApJ...915...92T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/915/92</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/J/A+A/432/369">J/A+A/432/369 : Leiden Atomic and Molecular Database (LAMDA) (Schoeier+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/178/247">J/ApJS/178/247 : H{alpha} and [NII] survey in local 11 Mpc (Kennicutt+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/629">J/A+A/486/629 : Effective collision strengths for C II (Tayal, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2563">J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/1672">J/ApJ/703/1672 : Far-IR and H{alpha} fluxes in galaxies (Kennicutt+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/1569">J/ApJ/703/1569 : Radial distribution in SINGS gal. 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