A Quantitative Analysis of the Morphology of Star Formation in Galaxies at Different Redshifts

Bibcode
2008ASPC..390..489A
Azzollini, R.; Beckman, J. E.
Bibliographical reference

Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at Santiago del Teide, Tenerife, Spain. Edited by J. H. Knapen, T. J. Mahoney, and A. Vazdekis San Francisco: Astronomical Society of the Pacific, 2008., p.489

Advertised on:
6
2008
Number of authors
2
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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.
Type
Non-refereed

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