« Lyman alpha emission during and after reionization » |
Jordi Miralda Escude |
A powerful probe to the high-redshift universe is found in the detection of Lyman alpha photons produced by several processes: star formation, gas cooling, fluorescence of ionizing radiation, and scattering of the background ultraviolet continuum. I will discuss how Lyman alpha emitting galaxies can be used to study the epoch of reionization at z ~ 6, and other applications of Lyman alpha fluorescence at lower redshifts. |
vendredi 5 mars 2010 - 11:00 Salle des séminaires Évry Schatzman, Institut d'Astrophysique de Paris |
Page web du séminaire / Seminar's webpage |