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Hiroyuki Hirashita

Identifiers

  • name variant Hiroyuki Hirashita 0.60 · backfill

Papers (53)

  1. Radiation-pressure-driven dust transport to galaxy halos at $z\sim 10$ astro-ph.GA · 2019 · author #1
  2. Dust scaling relations in a cosmological simulation astro-ph.GA · 2019 · author #3
  3. Remodeling the evolution of grain size distribution in galaxies astro-ph.GA · 2018 · author #1
  4. Comparison of cosmological simulations and deep submillimetre galaxy surveys astro-ph.GA · 2018 · author #2
  5. Cosmological simulation with dust formation and destruction astro-ph.GA · 2018 · author #3
  6. Exploring the Dust Population in Cold Diffuse Clouds astro-ph.GA · 2017 · author #2
  7. Populating H$_2$ and CO in galaxy simulation with dust evolution astro-ph.GA · 2017 · author #2
  8. Dust masses of $z>5$ galaxies from SED fitting and ALMA upper limits astro-ph.GA · 2017 · author #1
  9. Evolution of dust extinction curves in galaxy simulation astro-ph.GA · 2017 · author #2
  10. Dust evolution with active galactic nucleus feedback in elliptical galaxies astro-ph.GA · 2017 · author #1
  11. Effects of dust evolution on the abundances of CO and H$_2$ astro-ph.GA · 2017 · author #1
  12. Galaxy Simulation with Dust Formation and Destruction astro-ph.GA · 2016 · author #4
  13. Dust evolution processes constrained by extinction curves in nearby galaxies astro-ph.GA · 2016 · author #2
  14. Millimeter-sized grains in the protostellar envelopes: where do they come from? astro-ph.SR · 2016 · author #2
  15. Revisiting the lifetime estimate of large presolar grains in the interstellar medium astro-ph.GA · 2016 · author #1
  16. First-generation Science Cases for Ground-based Terahertz Telescopes astro-ph.GA · 2015 · author #1
  17. Dust processing in elliptical galaxies astro-ph.GA · 2015 · author #1
  18. The origin of dust extinction curves with or without the 2175 A bump in galaxies: The case of the Magellanic Clouds astro-ph.GA · 2015 · author #2
  19. Dust Cooling in Supernova Remnants in the Large Magellanic Cloud astro-ph.GA · 2015 · author #3
  20. A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope astro-ph.HE · 2015 · author #4
  21. Two-size approximation: a simple way of treating the evolution of grain size distribution in galaxies astro-ph.GA · 2014 · author #1
  22. Evolution of grain size distribution in high-redshift dusty quasars: Integrating large amounts of dust and unusual extinction curves astro-ph.GA · 2014 · author #3
  23. Effects of grain growth on the interstellar polarization curve astro-ph.GA · 2014 · author #2
  24. Molecular hydrogen emission in the interstellar medium of the Large Magellanic Cloud astro-ph.GA · 2014 · author #17
  25. Constraining dust formation in high-redshift young galaxies astro-ph.GA · 2014 · author #1
  26. The dust production rate of AGB stars in the Magellanic Clouds astro-ph.GA · 2014 · author #6
  27. Evolution of dust content in galaxies probed by gamma-ray burst afterglows astro-ph.GA · 2014 · author #2
  28. Planet Traps and First Planets: the Critical Metallicity for Gas Giant Formation astro-ph.EP · 2014 · author #2
  29. Evolution of the extinction curves in galaxies astro-ph.GA · 2014 · author #3
  30. Dense molecular cloud cores as a source of micrometer-sized grains in galaxies astro-ph.GA · 2014 · author #1
  31. Formation History of Polycyclic Aromatic Hydrocarbons in Galaxies astro-ph.GA · 2014 · author #2
  32. Effects of grain growth mechanisms on the extinction curve and the metal depletion in the interstellar medium astro-ph.GA · 2013 · author #1
  33. Discovery of an Outstanding Disk in the cD Galaxy of the Hydra A Cluster astro-ph.GA · 2013 · author #6
  34. Condition for the formation of micron-sized dust grains in dense molecular cloud cores astro-ph.GA · 2013 · author #1
  35. What determines the grain size distribution in galaxies? astro-ph.GA · 2013 · author #3
  36. Evolution of dust grain size distribution by shattering in the interstellar medium: robustness and uncertainty astro-ph.GA · 2013 · author #1
  37. Dust formation history of galaxies: a critical role of metallicity for the dust mass growth by accreting materials in the interstellar medium astro-ph.GA · 2012 · author #3
  38. Impact of grain size distributions on the dust enrichment in high-redshift quasars astro-ph.GA · 2012 · author #2
  39. Dust properties in afterglow of GRB 071025 at z~5 astro-ph.CO · 2011 · author #6
  40. Central free-free-dominated 880 $\micron$ emission in II Zw 40 astro-ph.CO · 2011 · author #1
  41. Effects of grain size distribution on the interstellar dust mass growth astro-ph.CO · 2011 · author #1
  42. The Role of Dust in the Early Universe I : Protogalaxy Evolution astro-ph.GA · 2011 · author #5
  43. Importance of far-infrared mapping in a spiral galaxy: AKARI observation of M81 astro-ph.CO · 2010 · author #2
  44. Shattering by turbulence as a production source of very small grains astro-ph.GA · 2010 · author #1
  45. Detecting Lyman Alpha Emitters in the Sub-millimeter astro-ph.CO · 2009 · author #2
  46. Origin of Chromatic Features in Multiple Quasars -Variability, Dust, or Microlensing - astro-ph · 2007 · author #2
  47. Common Correlations between 60, 100 and 140 um Intensities in the Galactic Plane and Magellanic Clouds astro-ph · 2006 · author #5
  48. Search for high column density systems with gamma ray bursts astro-ph · 2006 · author #1
  49. A model for the infrared dust emission from forming galaxies astro-ph · 2005 · author #5
  50. Absorption Measurement of Hydrogen Molecules in the Early Universe astro-ph · 2001 · author #4
  51. H2 Formation in Low Metallicity Galaxies astro-ph · 2001 · author #2
  52. Effect of Dust Extinction on Estimating Star Formation Rate of Galaxies: Lyman Continuum Extinction astro-ph · 2001 · author #2
  53. Star Formation Efficiency in the Central 1 kpc Region of Early-Type Spiral Galaxies astro-ph · 2000 · author #2

Mentions

  • 1511.00839 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1509.03978 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1507.03327 #2 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1506.07926 #3 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1503.07594 #4 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1412.3866 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1410.7861 #3 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1408.4682 #2 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1407.7658 #17 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1406.6762 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1404.7132 #6 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1404.5724 #2 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1404.5462 #2 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1401.7121 #3 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1401.5570 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1401.3943 #2 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1310.4679 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1310.3349 #6 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1306.5575 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1303.5528 #3 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1303.3958 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1206.0817 #3 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1205.6137 #2 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1110.3259 #6 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1107.5902 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1105.4930 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1104.0728 #5 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1010.1419 #2 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 1006.2187 #1 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 0908.1571 #2 · backfill · confidence 0.70 Hiroyuki Hirashita
  • 0709.1527 #2 · backfill · confidence 0.70 Hiroyuki Hirashita

Frequent Coauthors