High molecular gas fractions in normal massive star-forming galaxies in the young Universe
about
A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34.An extremely young massive clump forming by gravitational collapse in a primordial galaxy.Pure iron grains are rare in the universeAstronomy. Let there be dust.A massive protocluster of galaxies at a redshift of z ≈ 5.3.The close environments of accreting massive black holes are shaped by radiative feedback.Ionization state of inter-stellar medium in galaxies: evolution, SFR–M*–Z dependence, and ionizing photon escapeHow supernova feedback turns dark matter cusps into coresGalaxy Zoo: CANDELS barred discs and bar fractionsLarge molecular gas reservoirs in ancestors of Milky Way-mass galaxies nine billion years agoThe KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typicalz∼ 1 star-forming galaxiesEarly Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies atz=2.0–4.7On the nature of Hα emitters atz∼ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequenceA survey of molecular gas in luminous sub-millimetre galaxiesThe merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS surveyUsing [C i] to probe the interstellar medium in z ∼ 2.5 sub-millimeter galaxies★A Herschel view of the far-infrared properties of submillimetre galaxiesThe LABOCA survey of the Extended Chandra Deep Field-South: clustering of submillimetre galaxiesThe properties of the star-forming interstellar medium atz = 0.84-2.23 from HiZELS: mapping the internal dynamics and metallicity gradients in high-redshift disc galaxiesSteady outflows in giant clumps of high-z disc galaxies during migration and growth by accretionDark-ages reionization and galaxy formation simulation – IX. Economics of reionizing galaxiesHigh-redshift major mergers weakly enhance star formationFrom cusps to cores: a stochastic modelA search for H i and OH absorption inz≳ 3 CO emittersExtragalactic Astronomy: From Pioneers to Big ScienceIn Pursuit of High Redshift GalaxiesResolved star formation relations at high redshift from the IRAM PHIBSS programThe Evolution of Gas Content and Star Formation from z=3 to z=0Reconstructing the star formation history of the Milky Way disc(s) from chemical abundancesMolecular gas content in strongly lensedz~ 1.5−3 star-forming galaxies with low infrared luminositiesALMA detection of [C ii] 158μm emission from a strongly lensedz= 2.013 star-forming galaxyMolecular gas content in typical L* galaxies at z ∼ 1.5 − 3A gas-rich AGN near the centre of a galaxy cluster atz~ 1.4Cold gas in the inner regions of intermediate redshift clustersTowards a resolved Kennicutt-Schmidt law at high redshiftStar Formation Efficiency at Intermediate RedshiftGas fraction and star formation efficiency atz< 1.0Molecular Gas in Galaxies at all RedshiftsGalaxy evolution and star formation efficiency at 0.2 < z < 0.6AGN-driven quenching of star formation: morphological and dynamical implications for early-type galaxies
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High molecular gas fractions in normal massive star-forming galaxies in the young Universe
description
article publié dans la revue scientifique Nature
@fr
scientific article published in Nature
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wetenschappelijk artikel
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наукова стаття, опублікована в Nature в лютому 2010
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name
High molecular gas fractions i ...... galaxies in the young Universe
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High molecular gas fractions i ...... galaxies in the young Universe
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High molecular gas fractions i ...... galaxies in the young Universe
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High molecular gas fractions i ...... galaxies in the young Universe
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High molecular gas fractions i ...... galaxies in the young Universe
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High molecular gas fractions i ...... galaxies in the young Universe
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High molecular gas fractions i ...... galaxies in the young Universe
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A. Burkert
A. Shapley
A. Sternberg
J. Comerford
J. Gracia-Carpio
K. Shapiro
L. J. Tacconi
M. C. Cooper
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P304
P356
10.1038/NATURE08773
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P50
P577
2010-02-11T00:00:00Z
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1046729428
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P818
P819
2010Natur.463..781T