The very late-stage merger IC 4200:pre-elliptical or pre-spiral?

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dc.creatorSerra, P.
dc.creatorTrager, S. C.
dc.creatorvan der Hulst, J. M.
dc.creatorOosterloo, T. A.
dc.creatorMorganti, R.
dc.creatorvan Gorkom, J. H.
dc.date2005-09-13
dc.date.accessioned2026-07-07T02:18:38Z
dc.date.available2026-07-07T02:18:38Z
dc.descriptionRecent observations have revealed a class of unusually HI-rich early-type galaxies. By combining observations of their morphology, stellar populations and neutral hydrogen we aim to understand how these galaxies fit into the hierarchical formation paradigm. Here we present the result of our radio and optical observations of a test case galaxy, the E/S0 IC 4200.
dc.descriptionProceedings for the 5th Marseille International Cosmology Conference: The Fabulous Destiny of Galaxies. (2 pages)
dc.identifierhttps://arxiv.org/abs/astro-ph/0509350
dc.identifierhttp://arxiv.org/abs/astro-ph/0509350
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9561
dc.subjectAstrophysics
dc.titleThe very late-stage merger IC 4200:pre-elliptical or pre-spiral?
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