Thursday, July 1, 2010, 3:00 pm — Small Seminar Room, Bldg. 510
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, and fluorescence of ionizing radiation. 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.
Hosted by: Anze Slosar
6582 | INT/EXT | Events Calendar
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