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<ri:Resource created="2014-07-10T11:09:50Z" 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>CIG 340 (IC 2487) HI mapping</title><shortName>J/A+A/567/A56</shortName><identifier>ivo://CDS.VizieR/J/A+A/567/A56</identifier><altIdentifier>doi:10.26093/cds/vizier.35670056</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Scott T.C.</name></creator><creator><name>Sengupta C.</name></creator><creator><name>Verdes Montenegro L.</name></creator><creator><name>Bosma A.</name></creator><creator><name>Athanassoula E.,Sulentic J.</name></creator><creator><name>Espada D.</name></creator><creator><name>Yun M.S.</name></creator><creator><name>Argudo-Fernandez M.</name></creator><date role="Updated">2015-01-03T14:07:01Z</date><date role="Created">2014-07-10T11:09:50Z</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>radio-galaxies</subject><subject>h-i-line-emission</subject><description>HI kinematic asymmetries are common in late-type galaxies irrespective of environment, although the amplitudes are strikingly low in isolated galaxies. As part of our studies of the HI morphology and kinematics in isolated late-type galaxies we have chosen several very isolated galaxies from the AMIGA sample for HI mapping. We present here the results of HI mapping of CIG 340 (IC 2487) which was selected because its integrated HI spectrum has a very symmetric profile (A_flux_=1.03+/-0.02). Optical images of the galaxy hinted at a warped disk in contrast to the symmetric integrated HI spectrum profile. Our aim is to determine the extent to which the optical asymmetry is reflected in the resolved HI morphology and kinematics. Resolved 21-cm HI line mapping has been carried out using the Giant Metrewave Radio Telescope (GMRT). 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