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<ri:Resource created="2012-03-26T13:28:58Z" 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>Star formation in E/S0 galaxies</title><shortName>J/ApJ/708/841</shortName><identifier>ivo://CDS.VizieR/J/ApJ/708/841</identifier><altIdentifier>doi:10.26093/cds/vizier.17080841</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wei L.H.</name></creator><creator><name>Kannappan S.J.</name></creator><creator><name>Vogel S.N.</name></creator><creator><name>Baker A.J.</name></creator><date role="Updated">2017-09-19T14:21:09Z</date><date role="Created">2012-03-26T13:28:58Z</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>h-i-line-emission</subject><subject>spectroscopy</subject><subject>surveys</subject><description>Recent work has identified a population of low-redshift E/S0 galaxies that lie on the blue sequence in color versus stellar mass parameter space, where spiral galaxies typically reside. While high-mass blue-sequence E/S0s often resemble young merger or interaction remnants likely to fade to the red sequence, we focus on blue-sequence E/S0s with lower stellar masses (M_*_&lt;a fewx10^10^M_{sun}_), which are characterized by fairly regular morphologies and low-density field environments where fresh gas infall is possible. This population may provide an evolutionary link between early-type galaxies and spirals through disk regrowth. Focusing on atomic gas reservoirs, we present new GBT HI data for 27 E/S0s on both sequences as well as a complete tabulation of archival HI data for other galaxies in the Nearby Field Galaxy Survey. Normalized to stellar mass, the atomic gas masses for 12 of the 14 blue-sequence E/S0s range from 0.1 to &gt;1.0, demonstrating that morphological transformation is possible if the detected gas can be converted into stars. These gas-to-stellar mass ratios are comparable to those of spiral and irregular galaxies and have a similar dependence on stellar mass.</description><source format="bibcode">2010ApJ...708..841W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/708/841</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/VIII/77">VIII/77 : HI spectral properties of galaxies (Springob+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/73">VIII/73 : HI Parkes All Sky Survey Catalogue (HIPASS) (Meyer+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/238">VII/238 : HYPERLEDA. 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