Statistics – Methodology
Scientific paper
Jun 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..390..489a&link_type=abstract
Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at S
Statistics
Methodology
Scientific paper
Here, we present briefly the methodology we have implemented to study the spatial distribution of massive star formation in galaxies. To do this, we analyze a sample of 759 galaxies in a range of redshifts extending up to z˜ 1. We use data from different surveys, which span in wavelength from FUV to NIR (GALEX, COMBO17, and GOODS-HST). The aim is to develop methodology which can be used to help decide between different basic models of galaxy formation using the spatial distribution of star formation within galaxies as the test parameter. In situ knowledge of the star formation distribution as a function of redshift will be a valuable counterpart to population synthesis studies, which at best integrate this kind of information over long periods.
Azzollini Ruyman
Beckman John E.
No associations
LandOfFree
A Quantitative Analysis of the Morphology of Star Formation in Galaxies at Different Redshifts 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 A Quantitative Analysis of the Morphology of Star Formation in Galaxies at Different Redshifts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Quantitative Analysis of the Morphology of Star Formation in Galaxies at Different Redshifts will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1244404