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<ri:Resource created="2017-03-29T14:06:44Z" 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>Emission-line spectroscopy in NGC 891</title><shortName>J/ApJ/832/118</shortName><identifier>ivo://CDS.VizieR/J/ApJ/832/118</identifier><altIdentifier>doi:10.26093/cds/vizier.18320118</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boettcher E.</name></creator><creator><name>Zweibel E.G.</name></creator><creator><name>Gallagher III J.S.</name></creator><creator><name>Benjamin R.A.</name></creator><date role="Updated">2017-12-15T10:55:38Z</date><date role="Created">2017-03-29T14:06:44Z</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>spectroscopy</subject><subject>interstellar-medium</subject><description>The observed scale heights of extraplanar diffuse ionized gas (eDIG) layers exceed their thermal scale heights by a factor of a few in the Milky Way and other nearby edge-on disk galaxies. Here, we test a dynamical equilibrium model of the eDIG layer in NGC 891, where we ask whether the thermal, turbulent, magnetic field, and cosmic-ray pressure gradients are sufficient to support the layer. In optical emission-line spectroscopy from the SparsePak integral field unit on the WIYN 3.5m telescope, the H{alpha} emission in position-velocity space suggests that the eDIG is found in a ring between galactocentric radii of R_min_&lt;=R&lt;=8kpc, where R_min_&gt;=2kpc. We find that the thermal ({sigma}_th_=11km/s) and turbulent ({sigma}_turb_=25km/s) velocity dispersions are insufficient to satisfy the hydrostatic equilibrium equation given an exponential electron scale height of h_z_=1.0kpc. Using a literature analysis of radio continuum observations from the CHANG-ES survey, we demonstrate that the magnetic field and cosmic-ray pressure gradients are sufficient to stably support the gas at R&gt;=8kpc if the cosmic rays are sufficiently coupled to the system ({gamma}_cr_=1.45). Thus, a stable dynamical equilibrium model is viable only if the eDIG is found in a thin ring around R=8kpc, and nonequilibrium models such as a galactic fountain flow are of interest for further study.</description><source format="bibcode">2016ApJ...832..118B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/832/118</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/II/249">II/249 : WHAM Northern Sky Survey, V-1.1 (Haffner+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/211">III/211 : Keck/HIRES Sky Line Atlas (Osterbrock+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/150/81">J/AJ/150/81 : CHANG-ES. IV. VLA D-configuration observations (Wiegert+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/575/A17">J/A+A/575/A17 : NGC 891 Herschel PACS and SPIRE spectroscopy (Hughes+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/565/A4">J/A+A/565/A4 : NGC 891 70-500um images (Hughes+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/396/1231">J/MNRAS/396/1231 : Astrophotometric catalogue of NGC 891 (Rejkuba+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RMxAA/45.261">J/other/RMxAA/45.261 : Diffuse ionized gas database DIGEDA</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/383/487">J/ApJ/383/487 : Planetary nebulae as standard candles. VII. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MajAxis</name><description>[-64/183] Fiber offset along major axis (1)</description><unit>arcsec</unit><ucd>pos;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MinAxis</name><description>[-96/96] Fiber offset along minor axis (1)</description><unit>arcsec</unit><ucd>pos;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>IHa</name><description>[0/1987] H{alpha} intensity; 1e-17erg/s/cm^2^ (2)</description><unit>1e-20W.m**-2</unit><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_IHa</name><description>[0/6] Uncertainty in IHa</description><unit>1e-20W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigmaHa</name><description>[0/81] H{alpha} line width (2)</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_sigmaHa</name><description>[0/22] Uncertainty in sigmaHa</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigmaN2</name><description>[0/78] The [N II] 6583A line width (2)</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_sigmaN2</name><description>[0/17] Uncertainty in sigmaN2</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigmaS2a</name><description>[0/87] The [S II] 6716A line width (2)</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_sigmaS2a</name><description>[0/26] Uncertainty in sigmaS2a</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigmaS2b</name><description>[0/84] The [S II] 6731A line width (2)</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_sigmaS2b</name><description>[0/20] Uncertainty in sigmaS2b</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vel</name><description>[0/640] H{alpha} velocity centroid</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Simbad column added by the CDS</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Simbad column added by the CDS</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>