The simulated HI sky at low redshift

Astronomy and Astrophysics

Volumn 504, Issue 1, 2009, Pages 15-32

  Popping, A ^a,b   Dave R ^c   Braun, R ^b   Oppenheimer, B D ^c  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b CSIRO   (Australia)

^c UNIVERSITY OF ARIZONA   (United States)

Author keywords

Cosmology: Miscellaneous; Galaxies: Structure; Intergalactic medium

Indexed keywords

COLUMN DENSITY; COSMOLOGY: MISCELLANEOUS; DENSITY RATIO; EMISSION PROPERTIES; FAIR REPRESENTATION; FEEDBACK PROCESS; FILAMENTARY STRUCTURES; GALAXIES: STRUCTURE; GALAXY FORMATIONS; HYDRODYNAMIC SIMULATION; INTERGALACTIC MEDIUM; MASS FUNCTIONS; MOLECULAR HYDROGEN; NEUTRAL FRACTIONS; NEUTRAL HYDROGEN; RED SHIFT; SELF-SHIELDING; STATISTICAL PROPERTIES; THERMAL PRESSURE; TWO-POINT CORRELATION FUNCTION; WEALTH OF INFORMATION;

CLUSTER ANALYSIS; DISCRIMINANT ANALYSIS; FLUID DYNAMICS; GALAXIES; HYDRODYNAMICS; HYDROGEN; OPTICAL INSTRUMENTS; OPTICAL TELESCOPES; REGRESSION ANALYSIS; TELESCOPES;

COSMOLOGY;

EID: 70149111677     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911811     Document Type: Article

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