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<ri:Resource created="2008-10-07T14:25:33Z" status="active" updated="2025-09-09T14:13:26Z" 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>Spatial orientation of planetary nebulae</title><shortName>J/PASP/120/380</shortName><identifier>ivo://CDS.VizieR/J/PASP/120/380</identifier><altIdentifier>doi:10.26093/cds/vizier.61200380</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Weidmann W.A.</name></creator><creator><name>Diaz R.J.</name></creator><date role="Updated">2025-09-09T14:13:26Z</date><date role="Created">2008-10-07T14:25:33Z</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>planetary-nebulae</subject><description>We analyze the spatial orientation of a homogeneous sample of 440 elongated Planetary Nebulae (PNe) in order to determine the orientation of their apparent major axis with respect to the Milky Way plane. We present some important geometrical and statistical considerations that have been overlooked by previous works on the subject. The global distribution of galactic position angles (GPA) of PNe is quantitatively not very different from a random distribution of orientations in the Galaxy. Nevertheless, we find that there is at least one region on the sky, toward the Galactic center, where a weak correlation may exist between the orientation of the major axis of some PNe and the Galactic equator, with an excess of axes with GPA~100{deg}. Therefore, we confirm that extrinsic phenomena (i.e., global Galactic magnetic fields, shell compression from motion relative to the Interstellar Medium) do not determine the morphology of PNe on most of the sky, with a possible exception toward the Galactic center.</description><source format="bibcode">2008PASP..120..380W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/120/380</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/V/127">V/127 : MASH Catalogues of Planetary Nebulae (Parker+ 2006-2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/24">IV/24 : Catalogue of Galactic Planetary Nebulae (Kohoutek, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/84">V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+, 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/323/484">J/AN/323/484 : Accurate coordinates of Planetary Nebulae (Kohoutek+, 2002)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/120/380</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/120/380</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/120/380</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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