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

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概要

• 論文の詳細を見る
• Astronomical Society of Japanの論文
• 1997-12-01

著者

• SOFUE Yoshiaki

  Institute of Astronomy, The University of Tokyo

• TANIGUCHI Yoshiaki

  Astronomical Institute, Graduate School of Science, Tohoku University

• Arimoto N

  National Astronomical Observatory

• Arimoto Nobuo

  Institute Of Space And Astronautical Science

• Arimoto Nobuo

  Institute Of Astronomy Facult Of Science The University Of Tokyo

• Sofue Yoshiaki

  Institute Of Astronomy The University Of Tokyo

• Taniguchi Yoshiaki

  Astronomical Institute Faculty Of Science Tohoku University

• Ikuta Chisato

  Institute Of Astronomy School Of Science The University Of Tokyo

• Ikuta Chisato

  Institute Of Astronomy The University Of Tokyo

• Sofue Yoshiaki

  Institute Of Astronomy Faculty Of Science The University Of Tokyo

関連論文

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• New High-Redshift Galaxies at z = 5.8-6.5 in the Subaru Deep Field
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