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<ri:Resource created="2023-03-29T08:44:24Z" 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>NIR sp. of Class 0 protostars in Perseus and Orion</title><shortName>J/ApJ/921/110</shortName><identifier>ivo://CDS.VizieR/J/ApJ/921/110</identifier><altIdentifier>doi:10.26093/cds/vizier.19210110</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Laos S.</name></creator><creator><name>Greene T.P.</name></creator><creator><name>Najita J.R.</name></creator><creator><name>Stassun K.G.</name></creator><date role="Updated">2023-06-15T09:20:36Z</date><date role="Created">2023-03-29T08:44:24Z</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>infrared-astronomy</subject><subject>spectroscopy</subject><subject>star-forming-regions</subject><subject>molecular-clouds</subject><description>We present near-infrared K-band spectra for a sample of seven Class 0 protostars in the Perseus and Orion star-forming regions. We detect Br{gamma}, CO overtone, and H_2_ emission, features that probe the near-circumstellar environment of the protostar and reveal evidence of magnetospheric accretion, a hot inner disk atmosphere, and outflows, respectively. Comparing the properties of these features with those of Class I sources from the literature, we find that their Br{gamma} emission and CO emission are generally consistent in strength and velocity width. The Br{gamma} line profiles are broad and centrally peaked, with FWHMs of ~200km/s and wings extending to ~300km/s. The line ratios of our H_2_ emission features, which are spatially extended for some sources, are consistent with shock excitation and indicate the presence of strong jets or a disk wind. Within our small sample, the frequency of CO band emission (~67%) is high relative to that of Class I samples (~15%), indicating that Class 0 sources have high inner disk accretion rates, similar to those of the most actively accreting Class I sources. Collectively, our results suggest that Class 0 sources have similar accretion mechanisms to the more evolved classes, with strong organized stellar magnetic fields established at the earliest observable stage of evolution.</description><source format="bibcode">2021ApJ...921..110L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/921/110</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/356/1010">J/A+A/356/1010 : Ortho:para-H2 ratio in C and J shocks (Wilgenbus+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/365/90">J/A+A/365/90 : NIR H lines in TTS (Folha+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1145">J/AJ/130/1145 : YSO near-infrared properties (Doppmann+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/638/293">J/ApJ/638/293 : 1.1mm sources in the Perseus Molecular Cloud (Enoch+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/646/1009">J/ApJ/646/1009 : Structures of dust in Perseus molecular cloud (Kirk+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/387/954">J/MNRAS/387/954 : H2 imaging of NGC 1333, L1455, L1448 and B1 (Davis+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/181/321">J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/1214">J/AJ/140/1214 : NIR spectroscopic survey of class I YSOs (Connelley+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/31">J/AJ/144/31 : Spitzer+2MASS phot. of protostar cand. 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