Why Can We Detect the High-Redshift Quasar BR 1202-0725 in CO?

• Chisato Ikuta

• Nobuo Arimoto

• Yoshiaki Sofue

Bibliographic Information

Other Title

• Why Can We Detect the High-Redshift Qua

Abstract

コレクション : 国立国会図書館デジタルコレクション > デジタル化資料 > 雑誌

Journal

• Publications of the Astronomical Society of Japan

  Publications of the Astronomical Society of Japan 49 (6), 647-651, 1997-12

  Tokyo : Astronomical Society of Japan

Details

• CRID: 1520573330198896896
• NII Article ID: 10002598741
• NII Book ID: AA1082896X
• ISSN: 00046264
• NDL BIB ID: 4384247
• Web Site: https://ndlsearch.ndl.go.jp/books/R000000004-I4384247
• Text Lang: en
• NDL Source Classification:
  • ZM33(科学技術--宇宙科学)
• Data Source:
  • NDL
  • CiNii Articles