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<ri:Resource created="2022-04-07T09:31:55Z" 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>Stellar parameters of a Young Stellar Snake</title><shortName>J/ApJ/904/196</shortName><identifier>ivo://CDS.VizieR/J/ApJ/904/196</identifier><altIdentifier>doi:10.26093/cds/vizier.19040196</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tian H.-J.</name></creator><date role="Updated">2023-08-16T14:04:34Z</date><date role="Created">2022-04-07T09:31:55Z</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>open-star-clusters</subject><subject>ob-stars</subject><subject>young-stellar-objects</subject><subject>pre-main-sequence-stars</subject><subject>visible-astronomy</subject><subject>narrow-band-photometry</subject><subject>radial-velocity</subject><subject>proper-motions</subject><description>We report the discovery of a young (only 30-40Myr) snake-like structure (dubbed a stellar snake) in the solar neighborhood from Gaia DR2. The average distance of this structure is about 310pc from us. Both the length and width are over 200pc, but the thickness is only about 80pc. The snake has one tail and two dissolving cores, which can be clearly distinguished in the 6D phase space. The whole structure includes thousands of members with a total mass of larger than 2000M{sun} in a uniform population. The population is so young that it cannot be well explained with the classical theory of tidal tails. We therefore suspect that the snake is hierarchically primordial, rather than the result of dynamically tidal stripping, even if the snake is probably expanding. The coherent 5D phase information and the ages suggest that the snake was probably born in the same environment as the filamentary structure of Beccari et al. If so, the snake could extend the sky region of the Vela OB2 association by a factor of ~2 and supplement the census of its coeval structures. This finding is useful to understanding the history of the formation and evolution of the Vela OB2 complex. The age of the snake well matches with that of the Gould Belt. In the sky region of our interest, we detect one new open cluster, which is named Tian 1 in this work.</description><source format="bibcode">2020ApJ...904..196T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/904/196</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/117/354">J/AJ/117/354 : OB associations from Hipparcos (de Zeeuw+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/358/13">J/MNRAS/358/13 : Faint dwarfs in NGC 2547 (Jeffries+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/661/1119">J/ApJ/661/1119 : Spectroscopy in the 25 Ori group (Briceno+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/393/538">J/MNRAS/393/538 : Stellar association around gamma Vel (Jeffries+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/495/807">J/A+A/495/807 : Shape parameters for 650 open clusters (Kharchenko+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A53">J/A+A/558/A53 : Milky Way global survey star clusters. 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(Kharchenko+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A94">J/A+A/563/A94 : Kinematics of the Gamma Vel cluster (Jeffries+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/561/A142">J/A+A/561/A142 : Galactic extinction from SDSS BHB stars (Tian+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/618/A93">J/A+A/618/A93 : Gaia DR2 open clusters in the Milky Way (Cantat-Gaudin+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/626/A17">J/A+A/626/A17 : Young population in Vela-Puppis region (Cantat-Gaudin+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/621/A115">J/A+A/621/A115 : Vela OB2 members (Cantat-Gaudin+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/631/A166">J/A+A/631/A166 : Members of 5 cluster in Ori OB1a association (Kos+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/122">J/AJ/158/122 : Local structure &amp; star formation history of MW (Kounkel+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/870/32">J/ApJ/870/32 : Kinematics in young star clusters &amp; associations (Kuhn+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/245/32">J/ApJS/245/32 : Newly identified star clusters in Gaia DR2 (Liu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/621/L3">J/A+A/621/L3 : Hyades tidal tails with Gaia DR2 (Meingast+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/621/L2">J/A+A/621/L2 : Hyades tidal tails revealed by Gaia DR2 (Roeser+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/633/A99">J/A+A/633/A99 : Gaia DR2 open clusters in Milky Way. 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