J/A+A/562/A121ivo://CDS.VizieR/J/A+A/562/A121doi:10.26093/cds/vizier.35620121CDSComeron S.Salo H.Laurikainen E.Knapen J.H.Buta R.J.,Herrera-Endoqui M.Laine J.Holwerda B.W.Sheth K.Regan M.W.,Hinz J.L.Munoz-Mateo J.C.Gil de Paz A.Menedez-Delmestre K.,Seibert M.Mizusawa T.Kim T.Erroz-Ferrer S.Gadotti D.A.,Athanassoula E.Bosma A.Ho L.C.2017-06-19T07:58:00Z2014-07-25T12:24:22ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frstar-atlasesgalaxiescatalogsring-galaxiesinfrared-sourcesResonance rings and pseudorings (here collectively called "rings") are thought to be related to the gathering of material near dynamical resonances caused by non-axisymmetries in galaxy discs. Therefore, they are the consequence of secular evolution processes that redistribute material and angular momentum in discs. Their study may give clues on the formation and growth of bars and other disc non-axisymmetries. Our aims are to produce a Catalogue and an Atlas of the rings detected in the Spitzer Survey of Stellar Structure in Galaxies (S4G) and to conduct a statistical study of the data in the Catalogue. We traced the contours of rings previously identified by Buta et al. (in preparation) and fitted them with ellipses. We found the orientation of bars by studying the galaxy ellipse fits from S4G's Pipeline4. We used the galaxy orientation data obtained by S4G's Pipeline 4 to obtain intrinsic ellipticities and orientations of rings and the bars. ARRAKIS contains data on 724 ringed galaxies in the S4G. The frequency of resonance rings in the S4G is of 16+/-1% and 35+/-1% for outer and inner features, respectively. Outer rings are mostly found in Hubble stages -1<=T<=4. Inner rings are found in a broad distribution that covers the range -1<=T<=7. We confirm that outer rings have two preferred orientations, namely parallel and perpendicular to the bar. We confirm a tendency for inner rings to be oriented parallel to the bar, but we report the existence of a significant fraction (maybe as large as 50%) of inner features that have random orientations with respect to the bar. These misaligned inner rings are mostly found in late-type galaxies (T>=4). We find that the fraction of barred galaxies hosting outer (inner) rings is ~1.7 times (~1.3 times) that in unbarred galaxies. We confirm several results from previous surveys, as well as predictions from simulations of resonant rings and/or from manifold flux tube theory. We report that a significant fraction of inner rings in late-type galaxies have a random orientation with respect to the bar. This may be due to spiral modes decoupled from the bar dominating the Fourier amplitude spectrum at the radius of the inner ring. The fact that rings are only mildly favoured by bars suggests that those in unbarred galaxies either formed due to weak departures from the axisymmetry of the galactic potential or that they are born because of bars that have been destroyed after the ring formation.2014A&A...562A.121Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/562/A121CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/PASP/122/1397 : Spitzer Survey of Stellar Structure in Galaxies (Sheth+ 2010)J/ApJS/190/147 : Mid-IR galaxy morphology from S^4^G (Buta+, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/562/A121https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/562/A121http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/562/A121https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/562/A121https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/562/A121http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/562/A121GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/562/A121/catalog (Catalogue with the properties of rings and bars in Spitzer Survey of Stellar Structure in Galaxies (S^4^G) ringed galaxies (J/PASP/122/1397))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/562/A121/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/562/A121/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/562/A121/catalog?GETtext/xml+votable180.050000true23.201667-79.4738890.0055555555555555565/6965 6/697 739 2121 4149 4167 4178 4328 4359 4405 4446-4447 4511 4869 4891 4913 4953 4989 5006 5017 5024 5028 5061 5067 5075-5076 5091 5125 5134 5142 5190 5198 5200 5202 5288 5305 5307 5332 5399 5440 5463 5545 5572 5579 5581 5586 5589 5594 5610 5617 5623 5629 5631 5634-5635 5639 5715 5751 5774 5793 5796 5811 5848 5890 5961-5962 5975-5976 5982 5995 6003 6010 6034 6064 6087 6093 6095 6102 6123 6426 6623 7177 7188 7207 7214 7221 7225 7234 7241 7287 7374 7386 7393 7398 7442 7479 7485 7498 7515 7550 7584 7606 7655 7658-7659 7704 7941 7957 7982 7986 7997-7998 8011 8018 8024 8042 8084 8089 8128 8195-8197 8225 8228 8235 8256 8287 8320 8329 8331 8359 8376 8382 8458 8473 8492 8506 8723 8728-8729 8853 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28172-28173 28191 28200-28201 28234 28264 28294 28304 28348 28374 28381 28435 28463 28495 28498 28508 28515-28517 28521 28529 28579 28593 28612 28653 31345 31352 31360 31365 31369 31407 31454 31469 32439 32482 32793 32909 32983 33151 33242 33271 33646 33654 33920 33951 33954 33958 33962 34264 34273 34302 34334 34343 34352 34361 34404 34471 34493-34495 34531 34533-34534 34542 34545 34554 34674 34694 34701 35193 35287 35581 35691 35746 35923 35925 35929 35966 35993 35995 36081 36107 36131 36134-36135 36147 36151-36152 36229 36234 36240 36242 36250 36258 36261 36266 36276 36288 36302 36325 36328 36332 36380 36448 36450 36480 36609 36611 36684 36732 36796 36848 43881 43920 43953-43954 43956 43978 43995 44006 44011 44026-44027 44449 44461 44579 44582 44627 44635-44637 44660 44718 44741 44809 44817 44822 44835 44844 44848 44866 44945 45050 45054 45112 45178 45469 45471 45512 45558 45809 45905 45990 45997 46013 46062 46170 46175 46327 46363 46398-46399 46442 46477 46481 46491 46525 46564 46568 46577 46615 46651 46689 46738 46783 46812 46916 46984 47030 47047 47386 47456 47566 48193 48270 48283 48292 48462 48464 48484 48502 49010 49118https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/562/A121?format=asciiInfrareddefaultJ/A+A/562/A121/catalogCatalogue with the properties of rings and bars in Spitzer Survey of Stellar Structure in Galaxies (S^4^G) ringed galaxies (J/PASP/122/1397)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintn_NameSimbad column added by the CDSmeta.notecharNameGalaxy namemeta.id;meta.maincharNfNumber of features reported for this galaxymeta.numberintnullableDist? Distance to the galaxyMpcpos.distance;pos.heliocentricfloatnullableKindKind of feature (1)meta.code;src.morphcharDmajFeature major diameterarcminphys.angSizefloatDminFeature minor diameterarcminphys.angSizefloatPA[0/180] Major axis PA of the featuredegpos.posAngfloatDmaj0? Feature deprojected major diameterarcminphys.angSizefloatnullableDmin0? Feature deprojected minor diameterarcminphys.angSizefloatnullablenodes[0/180]? Deprojected major axis angle difference {theta}_r_ with respect to the line of nodes of the deprojectiondegpos.posAngfloatnullableS4GSimbad column added by the CDSmeta.idcharSimbadSimbad column added by the CDSmeta.ref.urlcharNEDSimbad column added by the CDSmeta.refchar_RAsource=J/PASP/122/1397/s4g Name= Position from the S4G (Sheth et al. 2010, Cat. J/PASP/122/1397) or Simbad (right ascension part)degpos.eq.ra;meta.main_DEsource=J/PASP/122/1397/s4g Name= Position from the S4G (Sheth et al. 2010, Cat. J/PASP/122/1397) or Simbad (declination part)degpos.eq.dec;meta.main