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<ri:Resource created="2013-06-19T08:39:16Z" 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>L1448 and HH211 CO(6-5) velocity maps</title><shortName>J/A+A/555/A8</shortName><identifier>ivo://CDS.VizieR/J/A+A/555/A8</identifier><altIdentifier>doi:10.26093/cds/vizier.35550008</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gomez-Ruiz A.I.</name></creator><creator><name>Wyrowski F.</name></creator><creator><name>Gusdorf A.</name></creator><creator><name>Leurini S.</name></creator><creator><name>Menten K.</name></creator><creator><name>Guesten R.</name></creator><date role="Updated">2017-03-20T07:38:33Z</date><date role="Created">2013-06-19T08:39:16Z</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><description>Observations of CO rotational transitions in the 0.3-0.4 millimeter range, now possible from exceptional sites on the ground, provide the opportunity of studing the warm component of molecular outflows in star-forming regions. This study aims to characterize the role of the warm gas in high-velocity and collimated outflows from Class 0 low-mass protostars. We used the CHAMP+ heterodyne array on the APEX telescope to map the CO (6-5) and CO (7-6) emission in the well-known Class 0 outflows L1448-mm and HH211-mm. We complement these data with ^13^CO (6-5) observations and also with previous low-J CO observations. The CO (6-5) and (7-6) emission was detected to be tracing the outflow lobes. In L1448, extremely high-velocity (EHV) emission was detected in both transitions. In HH211, high-velocity CO (6-5) emission was detected to be tracing the regions close to the central object, but it was also found close to the bow-shock regions seen in the mid-IR. A large velocity gradient code applied to these and the complementary low-J CO data revealed the high-velocity components to be dense (10^5^cm^-3) and warm (T&gt;200K) gas, in agreement with previous observations of shock tracers such as SiO. The high-velocity emission of these mid-J CO transitions are very good tracers of the inner highly excited part of outflows, which possibly is molecular material related to the underlying jet. 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