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Structure and Evolution of Nearby UV-bright Starburst Galaxies

J. S. Gallagher·C. J. Conselice·N. Homeier·The WFPC2 Investigation Definition Team
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Abstract

Nearby (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.

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J. S. Gallagher, C. J. Conselice, N. Homeier, The WFPC2 Investigation Definition Team. 1999-10-22. Structure and Evolution of Nearby UV-bright Starburst Galaxies. https://arxiv.org/abs/astro-ph/9910405

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