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<ri:Resource created="2023-03-14T12:28:11Z" 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>SDSS shocked post-starburst gal. with HST obs.</title><shortName>J/ApJ/919/134</shortName><identifier>ivo://CDS.VizieR/J/ApJ/919/134</identifier><altIdentifier>doi:10.26093/cds/vizier.19190134</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sazonova E.</name></creator><creator><name>Alatalo K.</name></creator><creator><name>Rowlands K.</name></creator><creator><name>Deustua S.E.</name></creator><creator><name>French K.D.,Heckman T.</name></creator><creator><name>Lanz L.</name></creator><creator><name>Lisenfeld U.</name></creator><creator><name>Luo Y.</name></creator><creator><name>Medling A.</name></creator><creator><name>Nyland K.,Otter J.A.</name></creator><creator><name>Petric A.O.</name></creator><creator><name>Snyder G.F.</name></creator><creator><name>Urry C.M.</name></creator><date role="Updated">2023-05-26T09:13:42Z</date><date role="Created">2023-03-14T12:28:11Z</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>hst-photometry</subject><subject>galaxy-classification-systems</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>infrared-photometry</subject><subject>ultraviolet-astronomy</subject><description>How do galaxies transform from blue, star-forming spirals to red, quiescent early-type galaxies? To answer this question, we analyzed a set of 26 gas-rich, shocked post-starburst galaxies with Hubble Space Telescope (HST) imaging in B, I, and H bands and Sloan Digital Sky Survey (SDSS) i-band imaging of similar depth but lower resolution. We found that post-starbursts in our sample have intermediate morphologies between disk- and bulge-dominated (Sersic n=1.7_-0.0_^+0.3^) and have red bulges, likely due to dust obscuration in the cores. A majority of galaxies in our sample are more morphologically disturbed than regular galaxies (88%, corresponding to &gt;3{sigma} significance) when observed with HST, with asymmetry and Sersic residual flux fraction being the most successful measures of disturbance. Most disturbances are undetected at the lower resolution of SDSS imaging. Although ~27% galaxies are clear merger remnants, we found that disturbances in another ~30% of the sample are internal, caused by small-scale perturbations or dust substructures rather than tidal features, and require high-resolution imaging to detect. We found 2.8{sigma} evidence that asymmetry features fade on timescales ~200Myr, and may vanish entirely after ~750Myr, so we do not rule out a possible merger origin of all post-starbursts given that asymmetric features may have already faded. This work highlights the importance of small-scale disturbances, detected only in high-resolution imaging, in understanding structural evolution of transitioning galaxies.</description><source format="bibcode">2021ApJ...919..134S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/919/134</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/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/342">II/342 : Hubble Source Catalog (V1 and V2) (Whitmore+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/342">II/342 : Hubble Source Catalog (V1 and V2) (Whitmore+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/335">II/335 : Revised catalog of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/107/1">J/ApJS/107/1 : Morphologies of distant galaxies II (Abraham+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/147/1">J/ApJS/147/1 : Classification of nearby galaxies (Conselice+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/163">J/AJ/128/163 : Galaxy morphological classification (Lotz+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/321">J/AJ/132/321 : Morphology of narrow-line Seyfert 1 galaxies (Deo+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/783">J/MNRAS/405/783 : Passive red spirals in Galaxy Zoo (Masters+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/411/2439">J/MNRAS/411/2439 : Coma Treasury Survey. 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