Metal-line emission from the warm-hot intergalactic medium - II. Ultraviolet

Monthly Notices of the Royal Astronomical Society

Volumn 408, Issue 2, 2010, Pages 1120-1138

  Bertone, Serena ^a   Schaye, Joop ^b   Booth, C M ^b   Vecchia, Claudio Dalla ^b,c   Theuns, Tom ^d,e   Wiersma, Robert P C ^b,f  

^a UNIVERSITY OF CALIFORNIA SANTA CRUZ   (United States)

^b LEIDEN UNIVERSITY   (Netherlands)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^d DURHAM UNIVERSITY   (United Kingdom)

^e UNIVERSITY OF ANTWERP   (Belgium)

^f MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Cosmology: theory; Diffuse radiation; Galaxies: formation; Intergalactic medium; Methods: numerical; Radiation mechanisms: thermal

Indexed keywords

BUDGET CONTROL; COSMOLOGY; DENSITY OF GASES; GALAXIES; GASES; HADRONS; LUMINANCE; METALS; NUMERICAL METHODS; SILICON CARBIDE;

COSMOLOGY: THEORY; DIFFUSE RADIATION; EMISSION LINES; GALAXY FORMATIONS; INTERGALACTIC MEDIUM; METAL LINE; METHOD: NUMERICAL; RADIATION MECHANISM: THERMAL; SURFACE BRIGHTNESS; WARM-HOT INTERGALACTIC MEDIUMS;

ELECTROMAGNETIC WAVE EMISSION;

EID: 78649436430     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.17188.x     Document Type: Article

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