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<ri:Resource created="2015-06-25T12:32:42Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Internal proper motions in NGC2392</title><shortName>J/ApJ/798/129</shortName><identifier>ivo://CDS.VizieR/J/ApJ/798/129</identifier><altIdentifier>doi:10.26093/cds/vizier.17980129</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Garcia-Diaz MA.T.</name></creator><creator><name>Gutierrez L.</name></creator><creator><name>Steffen W.</name></creator><creator><name>Lopez J.A.</name></creator><creator><name>Beckman J.</name></creator><date role="Updated">2015-07-19T14:48:12Z</date><date role="Created">2015-06-25T12:32:42Z</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><subject>proper-motions</subject><subject>radial-velocity</subject><description>We present measurements of internal proper motions at more than 500 positions of NGC 2392, the Eskimo Nebula, based on images acquired with WFPC2 on board the Hubble Space Telescope at two epochs separated by 7.695yr. Comparisons of the two observations clearly show the expansion of the nebula. We measured the amplitude and direction of the motion of local structures in the nebula by determining their relative shift during that interval. In order to assess the potential uncertainties in the determination of proper motions in this object, in general, the measurements were performed using two different methods, used previously in the literature. We compare the results from the two methods, and to perform the scientific analysis of the results we choose one, the cross-correlation method, because it is more reliable. We go on to perform a "criss-cross" mapping analysis on the proper motion vectors, which helps in the interpretation of the velocity pattern. By combining our results of the proper motions with radial velocity measurements obtained from high resolution spectroscopic observations, and employing an existing 3D model, we estimate the distance to the nebula to be 1.3kpc.</description><source format="bibcode">2015ApJ...798..129G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/798/129</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/714/1096">J/ApJ/714/1096 : Galactic planetary nebulae (Stanghellini+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/689/194">J/ApJ/689/194 : Distances of galactic planetary nebulae (Stanghellini+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/33/657">J/PAZh/33/657 : JHKLM photometry of eight planetary nebulae (Taranova+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/124/195">J/ApJS/124/195 : PN medium-resolution spectra (Hora+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/132/13">J/A+AS/132/13 : Planetary nebulae radial velocities (Durand+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/94/399">J/A+AS/94/399 : Absolute fluxes and distances of PN (Cahn+, 1992)</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/ApJ/798/129</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/798/129</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/798/129</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/798/129</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/798/129</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/798/129</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/798/129/table3</name><description>Proper motions of NGC 2392</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>X</name><description>[-22/29] Structure X axis position (4)</description><unit>arcsec</unit><ucd>pos.frame</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>[-26/24] Structure Y axis position (4)</description><unit>arcsec</unit><ucd>pos.frame</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmxp</name><description>Structure proper motion along X in pixels (2)</description><unit>pix</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmyp</name><description>Structure proper motion along Y in pixels (2)</description><unit>pix</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmxv</name><description>[-49.1/38.8] Structure proper motion along X in km/s (3)</description><unit>km/s</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmyv</name><description>[-35.4/48.7] Structure proper motion along Y in km/s (3)</description><unit>km/s</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pm</name><description>[0.01/69.3] Proper motion vector</description><unit>km/s</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RVel</name><description>[-49.4/165] Radial velocity (1)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>