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<ri:Resource created="2012-12-19T08:44:51Z" 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>Galaxy bulge types within 11Mpc</title><shortName>J/ApJ/733/L47</shortName><identifier>ivo://CDS.VizieR/J/ApJ/733/L47</identifier><altIdentifier>doi:10.26093/cds/vizier.17339047</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fisher D.B.</name></creator><creator><name>Drory N.</name></creator><date role="Updated">2018-01-08T06:38:07Z</date><date role="Created">2012-12-19T08:44:51Z</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>catalogs</subject><subject>galaxy-classification-systems</subject><description>We present an inventory of galaxy bulge types (elliptical galaxy, classical bulge, pseudobulge, and bulgeless galaxy) in a volume-limited sample within the local 11Mpc sphere using Spitzer 3.6um and Hubble Space Telescope data. We find that whether counting by number, star formation rate, or stellar mass, the dominant galaxy type in the local universe has pure disk characteristics (either hosting a pseudobulge or being bulgeless). Galaxies that contain either a pseudobulge or no bulge combine to account for over 80% of the number of galaxies above a stellar mass of 10^9^M_{sun}_. Classical bulges and elliptical galaxies account for ~1/4, and disks for ~3/4 of the stellar mass in the local 11Mpc. About 2/3 of all star formation in the local volume takes place in galaxies with pseudobulges. Looking at the fraction of galaxies with different bulge types as a function of stellar mass, we find that the frequency of classical bulges strongly increases with stellar mass, and comes to dominate above 10^10.5^M_{sun}_. Galaxies with pseudobulges dominate at 10^9.5^-10^10.5^M_{sun}_. Yet lower-mass galaxies are most likely to be bulgeless. If pseudobulges are not a product of mergers, then the frequency of pseudobulges in the local universe poses a challenge for galaxy evolution models.</description><source format="bibcode">2011ApJ...733L..47F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/733/L47</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/VII/155">VII/155 : Third Reference Cat. of Bright Galaxies (RC3) (de Vaucouleurs+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/196/11">J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/942">J/ApJ/716/942 : Bulges of nearby galaxies with Spitzer (Fisher+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/216">J/ApJS/182/216 : Surface photometry of Virgo ellipticals (Kormendy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/706/599">J/ApJ/706/599 : H{alpha} and UV SFR in the local volume (Lee+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/1672">J/ApJ/703/1672 : Far-IR and H{alpha} fluxes in galaxies (Kennicutt+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/773">J/AJ/136/773 : Structure of classical bulges and pseudobulges (Fisher+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/178/247">J/ApJS/178/247 : H{alpha} and [NII] survey in local 11 Mpc (Kennicutt+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2782">J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/145/405">J/A+AS/145/405 : Box- and peanut-shaped bulges. 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