The intergalactic medium near high-redshift galaxies

Details The intergalactic medium near high-redshift galaxies The intergalactic medium near high-redshift galaxies

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012phdt.........1r&link_type=abstract

Ph. D. thesis, University of Leiden (2012). Advisors: J. Schaye, C.C. Steidel, P.T. de Zeeuw. ISBN: 9789461911681

Astronomy and Astrophysics

Astronomy

Galaxies, High-Redshift Galaxies, Intergalactic Medium, Natal Galaxies

Scientific paper

Over the past 15 years, the field of extragalactic astronomy has pushed to high redshift and our knowledge of natal galaxies has grown dramatically. Galaxies are now routinely detected at redshifts z ! 6-7 (e.g. Bouwens et al. 2010; Labbé et al. 2010; Oesch et al. 2010; Bouwens et al. 2011; McLure et al. 2011). However, there are fundamental concepts that are still poorly understood. How do galaxies get their gas? How does galactic feedback affect galaxy evolution?

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