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<ri:Resource created="2005-06-12T17:22:08Z" 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>Galaxies with rows</title><shortName>J/AZh/78/963</shortName><identifier>ivo://CDS.VizieR/J/AZh/78/963</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chernin A.D.</name></creator><creator><name>Kravtsova A.S.</name></creator><creator><name>Zasov A.V.</name></creator><creator><name>Arkhipova V.P.</name></creator><date role="Updated">2017-12-22T05:32:09Z</date><date role="Created">2005-06-12T17:22:08Z</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>The results of a search for galaxies with straight structural elements, usually spiral-arm rows ("rows" in the terminology of Vorontsov-Vel'yaminov), are reported. The list of galaxies that possess (or probably possess) such rows includes about 200 objects, of which about 70% are brighter than 14m. On the whole, galaxies with rows make up 6-8% of all spiral galaxies with well-developed spiral patterns. Most galaxies with rows are gas-rich Sbc-Scd spirals. The fraction of interacting galaxies among them is appreciably higher than among galaxies without rows. Earlier conclusions that, as a rule, the lengths of rows are similar to their galactocentric distances and that the angles between adjacent rows are concentrated near 120{deg} are confirmed. 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HI mass-to-light ratio</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rows</name><description>Number of rows detected in the galaxy</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VV</name><description>? VV number (Vorontsov-Vel'Yaminov, 1977A&amp;AS...28....1V)</description><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>n_VV</name><description>[*] *: interacting galaxies with no VV numbers</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Com</name><description>Comments (1)</description><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>NED</name><description>Simbad column added by the CDS</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>