Do outflows from the high-mass star-forming regions favor MHD two-component structure?

Bibliographic Information

Other Title
  • 大質量星形成領域からのアウトフローは磁気流体「2成分」モデルを支持するか?

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Details 詳細情報について

  • CRID
    1573387449045312128
  • NII Article ID
    10004583831
  • NII Book ID
    AN00154555
  • ISSN
    03742466
  • Text Lang
    ja
  • Data Source
    • CiNii Articles

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