The nature of H i absorbers in gamma-ray burst afterglows: Clues from hydrodynamic simulations

Monthly Notices of the Royal Astronomical Society

Volumn 402, Issue 3, 2010, Pages 1523-1535

  Pontzen, Andrew ^a   Deason, Alis ^a   Governato, Fabio ^b   Pettini, Max ^a   Wadsley, James ^c   Quinn, Thomas ^b   Brooks, Alyson ^b,d   Bellovary, Jillian ^b   Fynbo, Johan P U ^e  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF WASHINGTON   (United States)

^c MCMASTER UNIVERSITY   (Canada)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e UNIVERSITY OF COPENHAGEN   (Denmark)

Author keywords

Galaxies: formation; Gamma rays: bursts; Quasars: absorption lines

Indexed keywords

ASTROPHYSICS; GALAXIES; GAMMA RAYS; HYDRODYNAMICS; METALS;

GALAXY FORMATIONS; GAMMA RAYS BURSTS; HIGH RESOLUTION SIMULATIONS; HIGH-REDSHIFT; HYDRODYNAMIC SIMULATION; MASSIVE STARS; METALLICITIES; PROPERTY; QUASARS ABSORPTION LINES; SPECTRA'S;

STARS;

EID: 77949335011     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.16017.x     Document Type: Article

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