Star formation trends in high-redshift galaxy surveys: the elephant or the tail?

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10 pages, 7 figures. Revised version: Fig. B2 removed after the discovery of an error, and Fig. 6 modified. Text and conclusio

Scientific paper

Star formation rate and accummulated stellar mass are two fundamental physical quantities that describe the evolutionary state of a forming galaxy. Two recent attempts to determine the relationship between these quantities, by interpreting a sample of star-forming galaxies at redshift of z~4, have led to opposite conclusions. We use a model galaxy population to investigate possible causes for this discrepancy and conclude that minor errors in the conversion from observables to physical quantities can lead to major misrepresentation when applied without awareness of sample selection. We also investigate, in a general way, the physical origin of the correlation between star formation rate and stellar mass within hierarchical galaxy formation theory.

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 trends in high-redshift galaxy surveys: the elephant or the tail? 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 trends in high-redshift galaxy surveys: the elephant or the tail?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star formation trends in high-redshift galaxy surveys: the elephant or the tail? will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-431599

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