Semi-analytic Model of Galaxy Formation in the Infrared: Predictions for SPICA

機関リポジトリ

この論文をさがす

説明

SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan

Understanding the galaxy dust emission is very important to obtain a full picture of galaxy formation, since it contains rich information about hidden star formation activity, physical properties of interstellar dust, and their role in galaxy formation. From the analysis of infrared spectral energy distribution (SED) of local galaxies which were observed by AKARI, we have found that a dust temperature averaged over the entire galaxy is strongly correlated with total infrared surface brightness, rather than total infrared luminosity. Combining this correlation with our cosmological galaxy formation model, we have computed dust SED of mock galaxies. By using this model, we present can theoretical predictions on the evolution of dusty universe.

形態: カラー図版あり

Physical characteristics: Original contains color illustrations

資料番号: AA1730027035

レポート番号: JAXA-SP-17-010E

収録刊行物

詳細情報 詳細情報について

  • CRID
    1050011086257272064
  • NII論文ID
    120006827242
  • ISSN
    24332232
  • Web Site
    http://id.nii.ac.jp/1696/00003006/
  • 本文言語コード
    en
  • 資料種別
    conference paper
  • データソース種別
    • IRDB
    • CiNii Articles

問題の指摘

ページトップへ