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Dust abundance and grain size in galaxy halos

  • Published:2020-04 Issue: Volume:183 Page:104504
  • ISSN:0032-0633
  • Container-title:Planetary and Space Science
  • language:en
  • Short-container-title:Planetary and Space Science

Author:

Hirashita Hiroyuki,Lin Chih-YuORCID

Funder

Ministry of Science and Technology

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference53 articles.

1. Intergalactic dust and observations of Type IA supernovae;Aguirre;Astrophys. J.,1999

2. Cosmological simulation with dust formation and destruction. ArXiv e-prints;Aoyama,2018

3. Galaxy simulation with dust formation and destruction;Aoyama;Mon. Not. Roy. Astron. Soc.,2017

4. What determines the grain size distribution in galaxies?;Asano;Mon. Not. Roy. Astron. Soc.,2013

5. Consistency among distance measurements: transparency, BAO scale and accelerated expansion;Avgoustidis;J. Cosmol. Astropart. Phys.,2009

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1. Evolution of grain size distribution in the circumgalactic medium;Publications of the Astronomical Society of Japan;2024-05-27

2. The survival and entrainment of molecules and dust in galactic winds;Monthly Notices of the Royal Astronomical Society;2024-04-27

3. On the Galactic Halos Rotation by Planck Data;Symmetry;2023-01-05

4. Shattering as a source of small grains in the circum-galactic medium;Monthly Notices of the Royal Astronomical Society;2021-05-17

5. The impact of astrophysical dust grains on the confinement of cosmic rays;Monthly Notices of the Royal Astronomical Society;2021-01-27
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