| 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 |