riassunto2

MG11 
Talk detail
 

 Participant 

Starling, Rhaana

Institution

Astronomical Institute 'Anton Pannekoek', University of Amsterdam  - Kruislaan 403 - Amsterdam - - THE NETHERLANDS

Session

Talk

Abstract

GRB3

Probing high redshift galaxies through optical afterglow spectra

Gamma-ray Bursts (GRBs) have been seen out to z=6.29. They enable the discovery of a population of distant, faint, star-forming galaxies in which they lie, not picked up by flux-limited surveys. Hence GRBs are a unique tool to probe cosmic chemical evolution and star-formation history. Absorption features imprinted on the bright optical afterglows reveal the conditions in the host galaxies. Metallicities, Z, spanning 0.01--0.1 Z_sun have now been measured in the spectra of several z>2 afterglows. Here I will discuss this exciting branch of GRB host studies and present 2 interesting cases in detail: GRB 060206 and GRB 050730.

 

Back to previous page