"Star formation in UV-bright interacting galaxies"

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dc.contributor.author Hulsebus, Alan
dc.contributor.author Nelson, Charles H.
dc.contributor.author Ragan, Sarah
dc.contributor.author McGleam, Catherine
dc.date.accessioned 2005-06-23T14:12:01Z
dc.date.available 2005-06-23T14:12:01Z
dc.date.issued 2005-06-23T14:12:01Z
dc.identifier.uri http://hdl.handle.net/2092/267
dc.description Alan Hulsebus is a Drake University student, majoring in Physics and Astronomy. Charles H. Nelson is Assistant Professor of Astronomy in the College of Arts and Sciences. He can be emailed at charles.nelson@drake.edu en
dc.description.abstract The interacting pair NGC3395 and NGC3396 and the interacting trio and NGC3991, NGC3994, and NGC3995 emit strongly in the ultraviolet, indicating multiple regions of active star formation. To investigate the nature of the star formation, we obtained U, B, V, and R images using the 40-inch telescope at Mt. Laguna. Our goal is to determine the sequence of star-formation episodes in these systems. Possibilities include a "chain reaction" - one burst triggering another burst and so on - or a continuity of stellar formation that remains approximately constant with time. en
dc.description.sponsorship Department of Physics and Astronomy, College of Arts and Sciences, Drake University. en
dc.format.extent 1161305 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.relation.ispartofseries DUCURS 2005;33
dc.subject Stars--Formation en
dc.subject Stars--Evolution en
dc.subject Galaxies en
dc.title "Star formation in UV-bright interacting galaxies" en
dc.type Presentation en


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  • DUCURS [193]
    Poster sessions and presentation from the Drake University Conference on Undergraduate Research in the Sciences held each April at Olmsted Center on the Drake campus.

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