Dust production 680-850 million years after the Big Bang

Abstract

Dust plays an important role in our understanding of the Universe, but it is not obvious yet how the dust in the distant universe was formed. I derived the dust yields per asymptotic giant branch (AGB) star and per supernova (SN) required to explain dust masses of galaxies at z=6.3-7.5 (680-850 million years after the Big Bang) for which dust emission has been detected (HFLS3 at z=6.34, ULAS J1120+0641 at z=7.085, and A1689-zD1 at z=7.5), or unsuccessfully searched for. I found very high required yields, implying that AGB stars could not contribute substantially to dust production at these redshifts, and that SNe could explain these dust masses, but only if they do not destroy most of the dust they form (which is unlikely given the upper limits on the SN dust yields derived for galaxies where dust is not detected). This suggests that the grain growth in the interstellar medium is likely required at these early epochs.

arXiv commentAccepted to A&A. 6 pages, 1 figure, 2 tables. V2: minor changes to match the published version

References in corpus (103)

• A luminous quasar at a redshift of z = 7.085
• A Cosmology Calculator for the World Wide Web
• The Galactic disk mass function: reconciliation of the HST and nearby determinations
• Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results
• Gas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range
• A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
• Dust Formation in Primordial Type II Supernovae
• Dust in the Early Universe: Dust Formation in the Ejecta of Population III Supernovae
• Dust Formation and Survival in Supernova Ejecta
• A dusty, normal galaxy in the epoch of reionization
• Herschel Detects a Massive Dust Reservoir in Supernova 1987A
• Evolution of interstellar dust and stardust in the solar neighbourhood
• A galaxy at a redshift z = 6.96
• A Redshift z = 6.56 Galaxy Behind the Cluster Abell 370
• A supernova origin for dust in a high-redshift quasar
• A Rapidly Star-forming Galaxy 700 Million Years After the Big Bang at z=7.51
• The Evolution of Dust in the Early Universe with Applications to the Galaxy SDSS J1148+5251
• Dust Formation In Early Galaxies
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• The Origin of Cosmic Dust
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• Stellar sources of dust in the high redshift Universe
• The global gas and dust budget of the Large Magellanic Cloud: AGB stars and supernovae, and the impact on the ISM evolution
• Rapid formation of large dust grains in the luminous supernova SN 2010jl
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• Dust Production and Particle Acceleration in Supernova 1987A Revealed with ALMA
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• Massive-Star Supernovae as Major Dust Factories
• A Herschel PACS and SPIRE study of the dust content of the Cassiopeia A supernova remnant
• An Intensely Star-Forming Galaxy at z~7 with Low Dust and Metal Content Revealed by Deep ALMA and HST Observations
• A Cool Dust Factory in the Crab Nebula: A Herschel Study of the Filaments
• The stellar masses and specific star-formation rates of submillimetre galaxies
• The origin of dust in high redshift QSOs: the case of SDSS J1148+5251
• Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC) II. Cool Evolved Stars
• Detection of atomic carbon [CII] 158 micron and dust emission from a z=7.1 quasar host galaxy
• The chemistry of population III supernova ejecta: II - The nucleation of molecular clusters as a diagnostic for dust in the early universe
• Discovery of a Giant Lya Emitter Near the Reionization Epoch
• Rapid dust production in submillimeter galaxies at z>4?
• The Origin of Dust in the Early Universe: Probing the Star Formation History of Galaxies by their Dust Content
• The Dust Budget of the SMC: Are AGB Stars the Primary Dust Source at Low Metallicity?
• Evolution of Thermally Pulsing Asymptotic Giant Branch Stars II. Dust production at varying metallicity
• The extinction law at high redshift and its implications
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• A Spitzer Space Telescope Study of SN 2003gd: Still No Direct Evidence that Core-Collapse Supernovae are Major Dust Factories
• Dust formation around AGB and SAGB stars: a trend with metallicity?
• The dust budget crisis in high-redshift submillimetre galaxies
• Spitzer Space Telescope Observations of Kepler's Supernova Remnant: A Detailed Look at the Circumstellar Dust Component
• The dust production rate of AGB stars in the Magellanic Clouds
• ALMA Observation of 158 micron [CII] Line and Dust Continuum of a z=7 Normally Star-forming Galaxy in the Epoch of Reionization
• Dust growth in the interstellar medium: How do accretion and coagulation interplay?
• Dust grain growth in the interstellar medium of 5<z<6.5 quasars
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• Dust Destruction in Type Ia Supernova Remnants in the Large Magellanic Cloud
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• New constraints on dust emission and UV attenuation of z=6.5-7.5 galaxies from millimeter observations
• Dust properties at z=6.3 in the host galaxy of GRB 050904
• Dust input from AGB stars in the Large Magellanic Cloud
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• The Importance of Physical Models for Deriving Dust Masses and Grain Size Distributions in Supernova Ejecta I: Radiatively Heated Dust in the Crab Nebula
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• Far-infrared and sub-mm observations of the Crab nebula
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• AKARI and BLAST Observations of the Cassiopeia A Supernova Remnant and Surrounding Interstellar Medium
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• The properties of the host galaxy and the immediate environment of GRB 980425 / SN 1998bw from the multi-wavelength spectral energy distribution
• The Detection of Cold Dust in Cas A: Evidence for the Formation of Metallic Needles in the Ejecta
• No evidence for dust extinction in GRB 050904 at z ~ 6.3
• A search for CII-158$\mu$m line emission in HCM\,6A, a Lyman-$\alpha$ emitter at $z=6.56$
• Properties of newly formed dust by SN2006jc based on near-to-mid infrared observation with AKARI
• Through the Looking Glass: Bright, Highly Magnified Galaxy Candidates at z~7 Behind Abell 1703
• Measuring Dust Production in the Small Magellanic Cloud Core-Collapse Supernova Remnant 1E 0102.2-7219
• Genesis and evolution of dust in galaxies in the early Universe II. Rapid dust evolution in quasars at z > 6
• GAMA/H-ATLAS: The Dust Opacity - Stellar Mass Surface Density Relation for Spiral Galaxies
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• AKARI Infrared Observations of the Supernova Remnant G292.0+1.8: Unveiling Circumstellar Medium and Supernova Ejecta
• Iron Needles in Supernova Remnants?

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