Structure and Evolution of Nearby UV-bright Starburst Galaxies

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dc.creatorGallagher, J. S.
dc.creatorConselice, C. J.
dc.creatorHomeier, N.
dc.creatorTeam, The WFPC2 Investigation Definition
dc.date1999-10-22
dc.date.accessioned2026-07-07T02:33:59Z
dc.date.available2026-07-07T02:33:59Z
dc.descriptionNearby (D < 100 Mpc) luminous blue starburst galaxies frequently show morphological evidence for recent involvement in mild collisions, or minor mergers where the disk survives. As a consequence UV-bright starbursts are preferentially seen in near face-on galaxies, and the postburst systems may become star-forming late-type galaxies. If this starburst evolutionary channel is important at moderate redshifts, then descendants of the faint blue galaxies could be the very common Sm-Sd field galaxies.
dc.description5 pages, Appearing in "Galaxy Dynamics: from the Early Universe to the Present", eds. F. Combes, G.A. Mamon, and V. Charmandaris
dc.identifierhttps://arxiv.org/abs/astro-ph/9910405
dc.identifierhttp://arxiv.org/abs/astro-ph/9910405
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15067
dc.subjectAstrophysics
dc.titleStructure and Evolution of Nearby UV-bright Starburst Galaxies
dc.typetext

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