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<ri:Resource created="2024-11-20T08:05:54Z" 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>Globular clusters from CFHT/MegaCam ugi obs. of M104</title><shortName>J/ApJ/939/74</shortName><identifier>ivo://CDS.VizieR/J/ApJ/939/74</identifier><altIdentifier>doi:10.26093/cds/vizier.19390074</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kang J.</name></creator><creator><name>Lee M.G.</name></creator><creator><name>Jang In S.</name></creator><creator><name>Ko Y.</name></creator><creator><name>Sohn J.</name></creator><creator><name>Hwang N.</name></creator><creator><name>Park B.-G.</name></creator><date role="Updated">2025-02-18T20:14:27Z</date><date role="Created">2024-11-20T08:05:54Z</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>galaxies</subject><subject>globular-star-clusters</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>two-color-diagrams</subject><description>M104 (NGC 4594, the Sombrero galaxy) is a mysterious massive early-type galaxy that shows a dominant bulge and a prominent disk. However, the presence of a halo in M104 has been elusive, and it is not yet known how M104 has acquired such a peculiar structure. Using wide (~2deg^2^) and deep ugi images of M104 obtained with the CFHT/MegaCam, we detect a large number of globular clusters (GCs) found out to R~35' (~100kpc). The color distribution of these GCs shows two subpopulations: a blue (metal-poor) system and a red (metal-rich) system. The total number of GCs is estimated to be N_GC_=1610+/-30 and the specific frequency to be SN=1.8+/-0.1. The radial number density profile of the GCs is steep in the inner region at R&lt;20' and becomes shallow in the outer region at 20'&lt;R&lt;35'. The outer region is dominated by blue GCs and is extended out to R~35'. This shows clearly the existence of a giant metal-poor halo in M104. The inner region is composed of a bulge hosting a disk, corresponding to a metal-rich halo as seen in early-type galaxies. At least two clumps of blue GCs are found in the outer region. One clump is overlapped with a faint stellar stream located in the southwest, indicating that it may be a remnant of a disrupted dwarf galaxy. Our results imply that the metal-rich inner halo of M104 formed first via major mergers, and the metal-poor outer halo grew via numerous minor mergers.</description><source format="bibcode">2022ApJ...939...74K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/939/74</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/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/195">VII/195 : Globular Clusters in the Milky Way (Harris, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/313/469">J/MNRAS/313/469 : Streaming motions of galaxy clusters. 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