Star Formation History and Other Properties of the Northern HDF

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Accepted by the Astrophysical Journal, 53 pages, 17 figures

Scientific paper

10.1086/378088

The original analysis of the star formation history in the NICMOS Deep images of the NHDF is extended to the entire NHDF utilizing NICMOS and WFPC2 archival data. The roughly constant star formation rate from redshifts 1 to 6 found in this study is consistent with the original results. Star formation rates from this study, Lyman break galaxies and sub-mm observations are now in concordance The spike of star formation at redshift 2 due to 2 ULIRGs in the small Deep NICMOS field is smoothed out in the larger area results presented here. The larger source base of this study allows comparison with predictions from hierarchical galaxy formation models. In general the observation are consistent with the predictions. The observed luminosity functions at redshifts 1-6 are presented for future comparisons with theoretical galaxy evolution calculations. Mid and far infrared properties of the sources are also calculated and compared with observations. A candidate for the VLA source VLA 3651+1221 is discussed.

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

Star Formation History and Other Properties of the Northern HDF 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 Star Formation History and Other Properties of the Northern HDF, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star Formation History and Other Properties of the Northern HDF will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-335920

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