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<ri:Resource created="2013-05-06T14:32:24Z" status="active" updated="2025-06-13T15:25:00Z" 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>Structure and dynamics of 8 low SB disc galaxies</title><shortName>J/MNRAS/423/962</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/423/962</identifier><altIdentifier>doi:10.26093/cds/vizier.74230962</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Morelli L.</name></creator><creator><name>Corsini E.M.</name></creator><creator><name>Pizzella A.</name></creator><creator><name>Dalla Bonta E.</name></creator><creator><name>Coccato L.,Mendez-Abreu J.</name></creator><creator><name>Cesetti M.</name></creator><date role="Updated">2024-07-18T20:18:35Z</date><date role="Created">2013-05-06T14:32:24Z</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>photometry</subject><subject>galaxy-classification-systems</subject><subject>chemical-abundances</subject><description>We present the radial profiles of the H{alpha}, Mg and Fe line-strength indices for a sample of eight spiral galaxies with a low-surface-brightness stellar disc and a bulge. The correlations between the central values of the line-strength indices and velocity dispersion are consistent with those known for early-type galaxies and bulges of high-surface-brightness galaxies. The age, metallicity and {alpha}/Fe enhancement of the stellar populations in the bulge-dominated region are obtained using stellar population models with variable element abundance ratios.</description><source format="bibcode">2012MNRAS.423..962M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/423/962</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/J/ApJS/105/209">J/ApJS/105/209 : Low surface brightness galaxies. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Galaxy name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType><flag>primary</flag></column><column><name>MType</name><description>Morphological classification (1)</description><ucd>src.morph</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>TT</name><description>Numerical morphological (typical error 1.0) (1)</description><ucd>src.morph</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Maj</name><description>Apparent isophotal diameter (2)</description><unit>arcmin</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Min</name><description>Apparent isophotal diameter (2)</description><unit>arcmin</unit><ucd>phys.angSize;src</ucd><dataType 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dispersion measured within an aperture of radius 0.3r_e_</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_sigma</name><description>rms uncertainty on sigma</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>&lt;Fe&gt;</name><description>Fe line-strength index measured within an aperture of radius 0.3r_e_</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_&lt;Fe&gt;</name><description>rms uncertainty on &lt;Fe&gt;</description><unit>0.1nm</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[MgFe]</name><description>Combined Mg-Fe line-strength index measured within an aperture of radius 0.3r_e_</description><unit>0.1nm</unit><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[MgFe]</name><description>rms uncertainty on [MgFe]</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mg2</name><description>Mg_2_ line-strength index measured within an aperture of radius 0.3r_e_</description><unit>mag</unit><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mg2</name><description>rms uncertainty on Mg2</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mgb</name><description>Mg_b_ line-strength index measured within an aperture of radius 0.3r_e_</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mgb</name><description>rms uncertainty on Mgb</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hb</name><description>H{beta} line-strength index measured within an aperture of radius 0.3r_e_</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Hb</name><description>rms uncertainty on Hb</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s</name><description>[1/2] Source of photometric and spectroscopic data: 1=Paper I (J/MNRAS/387/1099), 2=this paper</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Age</name><description>Mean age of the stellar population of the bulge</description><unit>Gyr</unit><ucd>time.age;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Age</name><description>rms uncertainty on 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