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<ri:Resource created="2016-04-05T12:43:22Z" 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>Spectra of CO and [CI] in protoplanetary disks</title><shortName>J/A+A/588/A108</shortName><identifier>ivo://CDS.VizieR/J/A+A/588/A108</identifier><altIdentifier>doi:10.26093/cds/vizier.35880108</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kama M.</name></creator><creator><name>Bruderer S.</name></creator><creator><name>Carney M.</name></creator><creator><name>Hogerheijde M.</name></creator><creator><name>van Dishoeck E.F.,Fedele D.</name></creator><creator><name>Baryshev A.</name></creator><creator><name>Boland W.</name></creator><creator><name>Gusten R.</name></creator><creator><name>Aikutalp A.</name></creator><creator><name>Choi Y.,Endo A.</name></creator><creator><name>Frieswijk W.</name></creator><creator><name>Karska A.</name></creator><creator><name>Klaassen P.</name></creator><creator><name>Koumpia E.</name></creator><creator><name>Kristensen L.,Leurini S.</name></creator><creator><name>Nagy Z.</name></creator><creator><name>Perez Beaupuits J.-P.</name></creator><creator><name>Risacher C.</name></creator><creator><name>van der Marel N.,van Kempen T.A.</name></creator><creator><name>van Weeren R.J.</name></creator><creator><name>Wyrowski F.</name></creator><creator><name>Yildiz U.A.</name></creator><date role="Updated">2017-06-13T11:14:42Z</date><date role="Created">2016-04-05T12:43:22Z</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>spectroscopy</subject><description>The gas-solid budget of carbon in protoplanetary disks is related to the composition of the cores and atmospheres of the planets forming in them. The principal gas-phase carbon carriers CO, C^0^, and C^+6 can now be observed regularly in disks. The gas-phase carbon abundance in disks has thus far not been well characterized observationally. We obtain new constraints on the [C]/[H] ratio in a large sample of disks, and compile an overview of the strength of [CI] and warm CO emission. We carried out a survey of the CO 6-5 line and the [CI] 1-0 and 2-1 lines towards 37 disks with the APEX telescope, and supplemented it with [CII] data from the literature. The data are interpreted using a grid of models produced with the DALI disk code. 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