{ "id": "2006.14314", "version": "v1", "published": "2020-06-25T11:29:13.000Z", "updated": "2020-06-25T11:29:13.000Z", "title": "Discovery of a near-infrared bar and a pseudobulge in the collisional ring galaxy Cartwheel", "authors": [ "Sudhanshu Barway", "Y. D. Mayya", "Aitor Robleto-OrĂºs" ], "comment": "Accepted for publication in MNRAS, 8 pages, 3 figures, 2 tables", "categories": [ "astro-ph.GA" ], "abstract": "We report the discovery of a bar, a pseudobulge and unresolved point source in the archetype collisional ring galaxy Cartwheel using careful morphological analysis of a near-infrared (NIR) K$_s$ band image of excellent quality (seeing=0.42\\arcsec) at the ESO archive. The bar is oval-shaped with a semi-major axis length of 3.23\\arcsec\\($\\sim$2.09~kpc), with almost a flat light distribution along it. The bulge is almost round (ellipticity=0.21) with an effective radius of 1.62\\arcsec\\ ($\\sim$1.05~kpc) and a Sersic index of 0.99, parameters typical of pseudobulges in late-type galaxies. The newly discovered bar is not recognisable as such in the optical images even with more than a factor of two higher spatial resolution of the Hubble Space Telescope, due to a combination of its red colour and the presence of dusty features. The observed bar and pseudobulge most likely belonged to the pre-collisional progenitor of the Cartwheel. The discovery of a bar in an archetype collisional ring galaxy Cartwheel is the first observational evidence to confirm the prediction that bars can survive a drop-through collision along with the morphological structures like a central bulge (pseudo).", "revisions": [ { "version": "v1", "updated": "2020-06-25T11:29:13.000Z" } ], "analyses": { "keywords": [ "pseudobulge", "near-infrared bar", "archetype collisional ring galaxy cartwheel", "semi-major axis length", "flat light distribution" ], "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable" } } }