Cosmic Dust - Near and Far

By Th. Henning, E. Grün, J. Steinacker. 2009

160 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/1f78073ab7aed0402d0e1fb2a94579ea83f3c937

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Citations in the corpus

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, methodology): “Liffman & Clayton 1989; Dwek 1998; Draine 2009; Jones & Nuth 2011). In these models, accretion of gas-phase metal onto dust grains becomes more efficient in dense molecular clouds as the ISM is metal-polluted by stellar ejecta and eventually increases the dust mass for fixed SFR (e.g. Asano et al. 2”
Modelling and interpreting spectral energy distributions of galaxies with BEAGLE (2016, background): “…is also that 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…”
THE CO-TO-H2 CONVERSION FACTOR FROM INFRARED DUST EMISSION ACROSS THE LOCAL GROUP (2011, background): “Meanwhile, accounting for the observed dust abundance appears to require buildup of dust in molecular clouds (Dwek 1998; Zhukovska et al. 2008; Draine 2009).”
Modelling the spectral energy distribution of galaxies - V. The dust and PAH emission SEDs of disk galaxies (2010, background): “Thirdly, the response of grains to light is not just a question of the wavelength and flux of the photons hitting them but alsoof their optical properties (dependent on shape, size and composition; see review by Draine 2010).”