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<ri:Resource created="2022-09-19T12:55:41Z" 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>Photometry and astrometry of M36 members</title><shortName>J/ApJ/910/80</shortName><identifier>ivo://CDS.VizieR/J/ApJ/910/80</identifier><altIdentifier>doi:10.26093/cds/vizier.19100080</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Panja A.</name></creator><creator><name>Chen W.P.</name></creator><creator><name>Dutta S.</name></creator><creator><name>Sun Y.</name></creator><creator><name>Gao Y.</name></creator><creator><name>Mondal S.</name></creator><date role="Updated">2023-08-16T14:50:42Z</date><date role="Created">2022-09-19T12:55:41Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><subject>proper-motions</subject><subject>stellar-distance</subject><description>We present comprehensive characterization of the Galactic open cluster M36. Some 200 member candidates, with an estimated contamination rate of ~8%, have been identified on the basis of proper motion and parallax measured by the Gaia DR2. The cluster has a proper motion grouping around ({mu}_{alpha}_cos{delta}=-0.15+/-0.01mas/yr, and {mu}_{delta}_=-3.35+/-0.02mas/yr), distinctly separated from the field population. Most member candidates have parallax values 0.7-0.9mas, with a median value of 0.82+/-0.07mas (distance ~1.20+/-0.13kpc). The angular diameter of 27'+/-0.4' determined from the radial density profile then corresponds to a linear extent of 9.42+/-0.14pc. With an estimated age of ~15Myr, M36 is free of nebulosity. To the southwest of the cluster, we discover a highly obscured (A_V_ up to ~23mag), compact (~1.9'x1.2') dense cloud, within which three young stellar objects in their infancy (ages &lt;~0.2Myr) are identified. The molecular gas, 3.6pc in extent, contains a total mass of (2-3)x10^2^M_{sun}_, and has a uniform velocity continuity across the cloud, with a velocity range of -20 to -22km/s, consistent with the radial velocities of known star members. In addition, the cloud has a derived kinematic distance marginally in agreement with that of the star cluster. If physical association between M36 and the young stellar population can be unambiguously established, this manifests a convincing example of prolonged star formation activity spanning up to tens of Myr in molecular clouds.</description><source format="bibcode">2021ApJ...910...80P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/910/80</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/I/297">I/297 : NOMAD Catalog (Zacharias+ 2005)</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/164">V/164 : LAMOST DR5 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/156">V/156 : LAMOST DR7 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/368">II/368 : The Spitzer (SEIP) source list (SSTSL2) (Spitzer Science Center, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/352/228">J/A+A/352/228 : Transitional YSOs candidates (Magnier+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/357/471">J/A+A/357/471 : BV and proper motions in NGC 1960 &amp; NGC 2194 (Sanner+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/80/8">J/AZh/80/8 : Proper motions of open star clusters (Loktin+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1916">J/AJ/126/1916 : JHK photometry of young clusters near the Sun (Porras+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/1669">J/AJ/132/1669 : Wide-field CCD phot. around nine open clusters (Sharma+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/468/151">J/A+A/468/151 : Nearby open clusters radii and masses (Piskunov+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/2340">J/AJ/134/2340 : Membership of Praesepe &amp; Coma Berenices (Kraus+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/118">J/AJ/136/118 : Open clusters as galactic disk tracers. 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