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dc.contributor.authorHulsebus, Alan
dc.contributor.authorNelson, Charles H.
dc.contributor.authorRagan, Sarah
dc.contributor.authorMcGleam, Catherine
dc.date.accessioned2005-06-23T14:12:01Z
dc.date.available2005-06-23T14:12:01Z
dc.date.issued2005-06-23T14:12:01Z
dc.identifier.urihttp://hdl.handle.net/2092/267
dc.descriptionAlan 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.eduen
dc.description.abstractThe 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.sponsorshipDepartment of Physics and Astronomy, College of Arts and Sciences, Drake University.en
dc.format.extent1161305 bytes
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.relation.ispartofseriesDUCURS 2005;33
dc.subjectStars--Formationen
dc.subjectStars--Evolutionen
dc.subjectGalaxiesen
dc.title"Star formation in UV-bright interacting galaxies"en
dc.typePresentationen


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  • DUCURS [196]
    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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