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<ri:Resource created="2018-04-17T12:56:30Z" 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>YSO jets from UWISH2. IV. Cygnus-X outflows</title><shortName>J/ApJS/234/8</shortName><identifier>ivo://CDS.VizieR/J/ApJS/234/8</identifier><altIdentifier>doi:10.26093/cds/vizier.22340008</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Makin S.V.</name></creator><creator><name>Froebrich D.</name></creator><date role="Updated">2018-05-17T12:17:01Z</date><date role="Created">2018-04-17T12:56:30Z</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>interstellar-medium</subject><subject>young-stellar-objects</subject><subject>infrared-photometry</subject><description>We have performed an unbiased search for outflows from young stars in Cygnus-X using 42deg^2^ of data from the UKIRT Widefield Infrared Survey for H_2_ (UWISH2 Survey), to identify shock-excited near-IR H_2_ emission in the 1-0 S(1) 2.122{mu}m line. We uncovered 572 outflows, of which 465 are new discoveries, increasing the number of known objects by more than 430%. This large and unbiased sample allows us to statistically determine the typical properties of outflows from young stars. We found 261 bipolar outflows, and 16% of these are parsec scale. The typical bipolar outflow is 0.45pc in length and has gaps of 0.025-0.1pc between large knots. The median luminosity in the 1-0 S(1) line is 10^-3^L_{sun}_. The bipolar flows are typically asymmetrical, with the two lobes misaligned by 5{deg}, one lobe 30% shorter than the other, and one lobe twice as bright as the other. Of the remaining outflows, 152 are single- sided and 159 are groups of extended, shock-excited H2 emission without identifiable driving sources. Half of all driving sources have sufficient WISE data to determine their evolutionary status as either protostars (80%) or classical T Tauri stars (20%). One-fifth of the driving sources are variable by more than 0.5mag in the K-band continuum over several years. Several of the newly identified outflows provide excellent targets for follow-up studies. We particularly encourage the study of the outflows and young stars identified in a bright-rimmed cloud near IRAS 20294+4255, which seems to represent a textbook example of triggered star formation.</description><source format="bibcode">2018ApJS..234....8M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/234/8</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/297">II/297 : AKARI/IRC mid-IR all-sky Survey (ISAS/JAXA, 2010)</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/II/316">II/316 : UKIDSS-DR6 Galactic Plane Survey (UGPS) (Lucas+ 2012)</relatedResource><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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/241/551">J/A+A/241/551 : Radio continuum in Cygnus X region (Wendker+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/392/239">J/A+A/392/239 : IR survey of outflows in Orion A (Stanke+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/472/187">J/A+A/472/187 : 12CO outflows towards submm cores in Per (Hatchell+, 2007)</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/A+A/496/153">J/A+A/496/153 : Molecular hydrogen flows along Ori A cloud (Davis+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/A24">J/A+A/511/A24 : MHO Catalogue (Davis+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/123">J/ApJS/188/123 : The Bolocam Galactic Plane Survey. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>OF</name><description>[001/599] Outflow number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MHO</name><description>MHO number(s) (1)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="125*">char</dataType></column><column><name>RAJ2000</name><description>[20] Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[36/45] Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Length1</name><description>[0.0007/0.07]? Length of outflow lobe 1 (2)</description><unit>deg</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Length2</name><description>[0.0005/0.09]? Length of outflow lobe 2</description><unit>deg</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PA1</name><description>[1/356]? Position angle of outflow lobe 1, degrees from north over east (2)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PA2</name><description>[174/360]? 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Integrated H_2_ flux of outflow lobe 2 at 2.122um (2)</description><unit>1e-19W.m**-2</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Cl*</name><description>[YN] Associated with star cluster or group?</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S</name><description>Outflow type (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Source</name><description>Candidate driving source identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="30*">char</dataType></column><column><name>CL</name><description>[0/95] Confidence level in driving source candidate</description><unit>%</unit><ucd>stat.fit.param;phys.atmol.level;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>JmagUG</name><description>[10.8/20.7]? 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