Imaging atomic and highly excited molecular gas in a z = 6.42 quasar host galaxy: copious fuel for an eddington-limited starburst at the end of cosmic reionization
about
Using [C i] to probe the interstellar medium in z ∼ 2.5 sub-millimeter galaxies★Production of dust by massive stars at high redshiftGenesis and evolution of dust in galaxies in the early UniverseGenesis and evolution of dust in galaxies in the early UniverseMolecular Gas in Galaxies at all RedshiftsGalaxy evolution and star formation efficiency at 0.2 < z < 0.6Discovery of an extremely bright submillimeter galaxy atz = 3.93CO(1–0) line imaging of massive star-forming disc galaxies at z=1.5–2.2Imaging the cold molecular gas in SDSS J1148 + 5251 at z = 6.4Very extended cold gas, star formation and outflows in the halo of a bright quasar atz> 6
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Imaging atomic and highly excited molecular gas in a z = 6.42 quasar host galaxy: copious fuel for an eddington-limited starburst at the end of cosmic reionization
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im September 2009 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
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wetenschappelijk artikel
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наукова стаття, опублікована у вересні 2009
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name
IMAGING ATOMIC AND HIGHLY EXCI ...... THE END OF COSMIC REIONIZATION
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Imaging atomic and highly exci ...... he end of cosmic reionization
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type
label
IMAGING ATOMIC AND HIGHLY EXCI ...... THE END OF COSMIC REIONIZATION
@nl
Imaging atomic and highly exci ...... he end of cosmic reionization
@en
prefLabel
IMAGING ATOMIC AND HIGHLY EXCI ...... THE END OF COSMIC REIONIZATION
@nl
Imaging atomic and highly exci ...... he end of cosmic reionization
@en
P2093
P50
P356
P1476
Imaging atomic and highly exci ...... he end of cosmic reionization
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P2093
Christopher L. Carilli
Karl M. Menten
Roberto Neri
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10.1088/0004-637X/703/2/1338
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P577
2009-09-09T00:00:00Z
P818
P819
2009ApJ...703.1338R