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Strangulation as the primary mechanism for shutting down star formation in galaxies.Ionization state of inter-stellar medium in galaxies: evolution, SFR–M*–Z dependence, and ionizing photon escapeEarly Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies atz=2.0–4.7Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMAMolecular hydrogen abundances of galaxies in the EAGLE simulationsMolecular gas content in strongly lensedz~ 1.5−3 star-forming galaxies with low infrared luminositiesPlanck intermediate results XLIII. Spectral energy distribution of dust in clusters of galaxiesStudying the evolution of AGB stars in theGaiaepochThe assembly of ‘normal’ galaxies atz ∼ 7 probed by ALMAObservational evidence of a slow downfall of star formation efficiency in massive galaxies during the past 10 GyrThe inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 <z< 3.0Mapping the average AGN accretion rate in the SFR–M* plane for Herschel★-selected galaxies at 0 < z ≤ 2.5Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy atz ~ 3.3Evidence for feedback in action from the molecular gas content in thez~ 1.6 outflowing QSO XID2028CO excitation of normal star-forming galaxies out to z = 1.5 as regulated by the properties of their interstellar mediumDust and gas in luminous proto-cluster galaxies at z = 4.05: the case for different cosmic dust evolution in normal and starburst galaxiesBlack hole accretion preferentially occurs in gas-rich galaxies*The rise and fall of stellar across the peak of cosmic star formation history: effects of mergers versus diffuse stellar mass acquisitionALLSMOG: an APEX Low-redshift Legacy Survey for MOlecular Gas – I. Molecular gas scaling relations, and the effect of the CO/H2 conversion factorThe Fundamental Plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulationsTriggering active galactic nuclei in hierarchical galaxy formation: disk instability vs. interactionsDust attenuation up to z ≃ 2 in the AKARI North Ecliptic Pole Deep FieldThe WISSH quasars projectRelative growth of black holes and the stellar components of galaxies
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P2860
description
article publié dans la revue scientifique Astronomy and Astrophysics
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im Februar 2014 veröffentlichter wissenschaftlicher Artikel
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scientific article published in Astronomy and Astrophysics
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wetenschappelijk artikel
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наукова стаття, опублікована в лютому 2014
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name
The evolution of the dust and gas content in galaxies
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The evolution of the dust and gas content in galaxies
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type
label
The evolution of the dust and gas content in galaxies
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The evolution of the dust and gas content in galaxies
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prefLabel
The evolution of the dust and gas content in galaxies
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The evolution of the dust and gas content in galaxies
@nl
P2093
P2860
P50
P356
P1476
The evolution of the dust and gas content in galaxies
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A. Grazian
D. J. Rosario
E. Le Floc’h
F. Mannucci
G. Granato
G. Li Causi
L. Riguccini
P2860
P356
10.1051/0004-6361/201322835
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P50
P577
2014-02-01T00:00:00Z
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P819
2014A&A...562A..30S