Dust destruction in the ISM: a re-evaluation of dust lifetimes

By A. Jones, J. Nuth. 2011

173 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/088dec5cc79cbb34592aef5be4f6f1e542296183

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In Astronomy and Astrophysics

Citations in the corpus

Modelling and interpreting spectral energy distributions of galaxies with BEAGLE (2016, background): “…this may be used to constrain the mechanisms of dust production (e.g. winds from asymptotic-giant-branch stars, supernova explosions; Höfner 2009; Cherchneff 2010) and destruction (e.g. shocks; Jones 2004; Jones & Nuth 2011) from the analysis of different types of galaxies at various redshifts.”
Production of dust by massive stars at high redshift (2011, background): “Estimates of grain lifetimes resulting from calculations for the Milky Way range between 100 and 1000 Myr(e.g., Jones et al, 1994), although these predictions are uncertain (e.g., Jones and Nuth, 2011).”
Dust formation history of galaxies: A critical role of metallicity* for the dust mass growth by accreting materials in the interstellar medium (2012, background): “In addition, we should consider the dust mass growth in the ISM by the accretion of atoms and molecules of refractory elements onto grains (e.g., Dwek, 1998; Liffman & Clayton, 1989; Draine, 2009; Jones & Nuth, 2011).”
DUST PRODUCTION AND PARTICLE ACCELERATION IN SUPERNOVA 1987A REVEALED WITH ALMA (2013, background): “However, dust formed in a supernova must survive passage through the reverse shock to be dispersed into the interstellar medium, and then also survive shock passages once dispersed (Jones & Nuth 2011).”
Detection of the Far-infrared [O iii] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era (2018, background): “In recent years, a microscopic process of grain growth in dense ISM has been studied to overcome the problem of explaining the high-z dust reservoirs (e.g., Liffman & Clayton 1989; Dwek 1998; Draine 2009; Jones & Nuth 2011).”
Astrophysics with Extraterrestrial Materials (2016, background): “This conclusion is tempered by the large uncertainties involved in the various timescale estimates and by the lack of a compelling mechanism for producing dust with the observed properties in the interstellar environment ( Jones & Nuth 2011).”
The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point (2013, background): “Based on earlier considerations (e.g., Jones et al. 1990; Jones 2001; Jones & Nuth 2011), the work of Köhler et al. (2011, 2012), Planck satellite observations (Planck Collaboration 2011b,a), and the optEC(s)(a) model data (Papers I to III), we suggest that the usual decomposition of the…”