Effects of grain size distribution on the interstellar dust mass growth

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Hirashita, Hiroyuki; Kuo, Tzu-Ming;
  • Related identifiers: doi: 10.1111/j.1365-2966.2011.19131.x
  • Subject: Astrophysics - Astrophysics of Galaxies | Astrophysics - Cosmology and Nongalactic Astrophysics
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics

Grain growth by the accretion of metals in interstellar clouds (called `grain growth') could be one of the dominant processes that determine the dust content in galaxies. The importance of grain size distribution for the grain growth is demonstrated in this paper. First... View more
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