Unveiling the physical properties of Lyman alpha emitters - constructing a theoretical model in the hierarchically clustering galaxy formation

Details Unveiling the physical properties of Lyman alpha emitters - constructing a theoretical model in the hierarchically clustering galaxy formation Unveiling the physical properties of Lyman alpha emitters - constructing a theoretical model in the hierarchically clustering galaxy formation

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008asthe.101...83k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 101, No. 2, p. 83 - 91 (2008)

Astronomy and Astrophysics

Astronomy

Galaxy Formation, Lyman-Alpha Emitters

Scientific paper

Detecting redshifted Lyman α emissions is a promising way to seek for high-z galaxies nowadays. While the number of Lyman α emitting galaxies (LAEs) has been increasing over the past decade, the question of what type of galaxies is observed as the LAEs remains open. The authors report a theoretical model for the LAE constructed to unveil its physical properties.

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