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<ri:Resource created="2015-05-19T13:57:45Z" 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>The SOS project. IV. NGC 1624 and NGC 1931</title><shortName>J/AJ/149/127</shortName><identifier>ivo://CDS.VizieR/J/AJ/149/127</identifier><altIdentifier>doi:10.26093/cds/vizier.51490127</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lim B.</name></creator><creator><name>Sung H.</name></creator><creator><name>Bessell M.S.</name></creator><creator><name>Kim J.S.</name></creator><creator><name>Hur H.</name></creator><creator><name>Park B.-G.</name></creator><date role="Updated">2015-06-24T21:12:45Z</date><date role="Created">2015-05-19T13:57:45Z</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>broad-band-photometry</subject><subject>h-alpha-photometry</subject><description>Young open clusters located in the outer Galaxy provide us with an opportunity to study star formation activity in a different environment from the solar neighborhood. We present a UBVI and H{alpha} photometric study of the young open clusters NGC 1624 and NGC 1931 that are situated toward the Galactic anticenter. Various photometric diagrams are used to select the members of the clusters and to determine the fundamental parameters. NGC 1624 and NGC 1931 are, on average, reddened by &lt;E(B-V)&gt;=0.92+/-0.05 and 0.74+/-0.17mag, respectively. The properties of the reddening toward NGC 1931 indicate an abnormal reddening law (R_V,cl_=5.2+/-0.3). Using the zero-age main sequence fitting method we confirm that NGC 1624 is 6.0+/-0.6kpc away from the Sun, whereas NGC 1931 is at a distance of 2.3+/-0.2kpc. The results from isochrone fitting in the Hertzsprung-Russell diagram indicate the ages of NGC 1624 and NGC 1931 to be less than 4 and 1.5-2.0Myr, respectively. We derived the initial mass function (IMF) of the clusters. The slope of the IMF ({Gamma}_NGC1624_=-2.0+/-0.2 and {Gamma}_NGC1931_=-2.0+/-0.1) appears to be steeper than that of the Salpeter/Kroupa IMF. We discuss the implication of the derived IMF based on simple Monte-Carlo simulations and conclude that the property of star formation in the clusters does not seem to be significantly different from that in the solar neighborhood.</description><source format="bibcode">2015AJ....149..127L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/149/127</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/B/ocl">B/ocl : Optically visible open clusters and Candidates (Dias+ 2002-2014)</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/J/MNRAS/438/1451">J/MNRAS/438/1451 : UBVIHa photometry of IC 1848 (Lim+, 2014; Paper II)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/172">J/ApJ/764/172 : UBVRI photometry of stars toward NGC 1931 (Pandey+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/46">J/AJ/145/46 : UBVIc photometry in Westerlund 1 (Lim+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/37">J/AJ/145/37 : UBVI and Ha CCD photometry of NGC 6231 (Sung+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/41">J/AJ/143/41 : UBVIc photometry of star clusters Tr14 and Tr16 (Hur+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/411/2530">J/MNRAS/411/2530 : UBVRIJHK photometry in NGC1624 (Jose+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/1116">J/AJ/138/1116 : A Spitzer view of NGC 2264 (Sung+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/441">J/AJ/135/441 : VRIHa photometry in NGC 2264 (Sung+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1684">J/AJ/128/1684 : NGC 2264: VRIHa photometry (Sung+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1014">J/AJ/127/1014 : CCD UBVRIHa photometry in NGC 3603 (Sung+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/120/333">J/AJ/120/333 : UBVRI and Ha in NGC 6530 (Sung+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/310/982">J/MNRAS/310/982 : UBVI CCD Photometry of M11 - II. 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