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dc.contributor.authorFrazier, Aaron G.
dc.contributor.authorNelson, Charles H.
dc.date.accessioned2005-06-23T14:27:49Z
dc.date.available2005-06-23T14:27:49Z
dc.date.issued2005-06-23T14:27:49Z
dc.identifier.urihttp://hdl.handle.net/2092/269
dc.descriptionAaron G. Frazier is a student at Drake University and Charles Nelson is Assistant Professor of Astronomy at Drake. He can be contacted at charles.nelson@drake.eduen
dc.description.abstractWe have obtained long-slit spectroscopy of the star-forming regions in NGC3395, NGC3396, 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 apporximately constant with time.en
dc.description.sponsorshipDrake University, College of Arts and Sciences, Department of Physics and Astronomy.en
dc.format.extent1096036 bytes
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.relation.ispartofseriesDUCURS 2005;32
dc.subjectStars--Formationen
dc.subjectStarburstsen
dc.subjectGalaxiesen
dc.title"Spectroscopy of star-forming regions in UV bright, interacting starburst 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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