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<ri:Resource created="2019-08-14T15:21:12Z" 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>H{alpha} &amp; UV emission scale heights for edge-on gal.</title><shortName>J/ApJ/862/25</shortName><identifier>ivo://CDS.VizieR/J/ApJ/862/25</identifier><altIdentifier>doi:10.26093/cds/vizier.18620025</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jo Y.-S.</name></creator><creator><name>Seon K.-I.</name></creator><creator><name>Shinn J.-H.</name></creator><creator><name>Yang Y.</name></creator><creator><name>Lee D.</name></creator><creator><name>Min K.-W.</name></creator><date role="Updated">2019-08-26T07:29:49Z</date><date role="Created">2019-08-14T15:21:12Z</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>ultraviolet-astronomy</subject><subject>visible-astronomy</subject><subject>interstellar-medium</subject><description>We compare vertical profiles of the extraplanar H{alpha} emission to those of the UV emission for 38 nearby edge-on late-type galaxies. It is found that detection of the "diffuse" extraplanar dust (eDust), traced by the vertically extended, scattered UV starlight, always coincides with the presence of the extraplanar H{alpha} emission. A strong correlation between the scale heights of the extraplanar H{alpha} and UV emissions is also found; the scale height at H{alpha} is found to be ~0.74 of the scale height at FUV. Our results may indicate the multiphase nature of the diffuse ionized gas and dust in the galactic halos. The existence of eDust in galaxies where the extraplanar H{alpha} emission is detected suggests that a larger portion of the extraplanar H{alpha} emission than that predicted in previous studies may be caused by H{alpha} photons that originate from HII regions in the galactic plane and are subsequently scattered by the eDust. This possibility raise an advantage in studying the extraplanar diffuse ionized gas. We also find that the scale heights of the extraplanar emissions normalized to the galaxy size correlate well with the star formation rate surface density of the galaxies. The properties of eDust in our galaxies is on a continuation line of that found through previous observations of the extraplanar polycyclic aromatic hydrocarbons emission in more active galaxies known to have galactic winds.</description><source format="bibcode">2018ApJ...862...25J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/862/25</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/109">VII/109 : IRAS Observations of Large Optical Galaxies (Rice+, 1988)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/141">VII/141 : Spectrophotometric Atlas of Galaxies (Kennicutt Jr. 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/312">II/312 : GALEX-DR5 (GR5) sources from AIS and MIS (Bianchi+ 2011)</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/A+A/414/23">J/A+A/414/23 : CCD H{alpha} and R photometry of 334 galaxies (James+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/165/307">J/ApJS/165/307 : Survey for ionization in neutral gas gal. 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