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<ri:Resource created="2014-04-11T09:12:12Z" 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>Chamaeleon-MMS1 NH_3_ (1,1) and (2,2) maps</title><shortName>J/A+A/564/A99</shortName><identifier>ivo://CDS.VizieR/J/A+A/564/A99</identifier><altIdentifier>doi:10.26093/cds/vizier.35640099</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Vaisala M.S.</name></creator><creator><name>Harju J.</name></creator><creator><name>Mantere M.J.</name></creator><creator><name>Miettinen O.</name></creator><creator><name>Sault R.S.,Walmsley C.M.</name></creator><creator><name>Whiteoak J.B.</name></creator><date role="Updated">2017-07-12T15:18:01Z</date><date role="Created">2014-04-11T09:12:12Z</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>young-stellar-objects</subject><subject>radio-astronomy</subject><description>The aim of this study is to investigate the structure and kinematics of the nearby candidate first hydrostatic core Cha-MMS1. Cha-MMS1 was mapped in the NH_3_(1,1) line and the 1.2cm continuum using the Australia Telescope Compact Array, ATCA. The angular resolution of the ATCA observations is 7" (~1000AU), and the velocity resolution is 50m/s. The core was also mapped with the 64-m Parkes telescope in the NH_3_(1,1) and (2,2) lines. Observations from Herschel Space Observatory and Spitzer Space telescope were used to help interpretation. The ammonia spectra were analysed using Gaussian fits to the hyperfine structure. 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