Computer Science
Scientific paper
May 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..408...45s&link_type=abstract
The ultraviolet universe at low and high redshift. AIP Conference Proceedings, Volume 408, pp. 45-49 (1997).
Computer Science
4
Starburst Galaxies And Infrared Excess Galaxies, Origin, Formation, Evolution, Age, And Star Formation, Ultraviolet
Scientific paper
Optical surveys for high-redshift (z~2-5) star forming galaxies will preferentially identify UV-bright systems since the observed optical emission corresponds to the rest-frame UV. Studies of nearby UV-bright starbursts thus provide a unique opportunity to obtain a detailed understanding of the phenomena observed at high redshifts. We discuss the far-ultraviolet (FUV; λ~1500 Å) properties of the nearby blue starburst galaxy NGC 3310. The FUV morphology is compared to that observed at longer wavelengths. The stellar content of selected star forming regions is also discussed.
Bohlin Ralph
Bothun Greg
Fanelli Michael N.
Neff Susan G.
O'Connell Robert West
No associations
LandOfFree
Ultraviolet imaging of nearby starbursts: NGC 3310 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Ultraviolet imaging of nearby starbursts: NGC 3310, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet imaging of nearby starbursts: NGC 3310 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-832934