Probing star formation at intermediate z

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Galaxies: Evolution, Galaxies: Starburst

Scientific paper

We summarize the latest results of an ongoing project aimed at connecting starburst galaxies in the local Universe and Lyman-break galaxies (LBGs) in the distant Universe using rest-frame ultraviolet (UV) images. We are quantifying star formation in the local Universe using GALEX data of interacting galaxies and we are using Hubble Space Telescope U-band and optical images of the Ultra Deep Field to quantify star formation at intermediate (z ~ 1) and high (z > 2) redshifts, respectively. We are measuring sizes of star-forming clumps in all redshift ranges and searching for evolutionary effects. We chose the rest-frame UV to do this work because young and massive stars radiate most their energy in the UV and also because LBGs are selected to be UV-bright. We discuss whether all galaxies go through an LBG phase and whether disks show any sign of size of evolution at z < 1.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Probing star formation at intermediate z 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 Probing star formation at intermediate z, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Probing star formation at intermediate z will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1448202

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.