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CO(3-2) Observations of IRAS F10214+4724 at NMA

Published online by Cambridge University Press:  12 April 2016

Sakamoto Kazushi ,
Kawabe Ryohei ,
Ishizuki Sumio  and
Ishiguro Masato
Sakamoto Kazushi
Affiliation:
Nobeyama Radio Observatory, Minamisaku, Nagano, 384-13, Japan Dept. of Astronomy, Univ. of Tokyo, Bunkyou, Tokyo, 113, JapanE-mail:sakamoto@nro.nao.ac.jp (INTERNET)
Kawabe Ryohei
Affiliation:
Nobeyama Radio Observatory, Minamisaku, Nagano, 384-13, Japan
Ishizuki Sumio
Affiliation:
Nobeyama Radio Observatory, Minamisaku, Nagano, 384-13, Japan Dept. of Astronomy, Univ. of Tokyo, Bunkyou, Tokyo, 113, JapanE-mail:sakamoto@nro.nao.ac.jp (INTERNET)
Ishiguro Masato
Affiliation:
Nobeyama Radio Observatory, Minamisaku, Nagano, 384-13, Japan

Abstract

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We have observed CO(J=3-2) emission of the z=2.286 galaxy IRAS F10214+4724 using the Nobeyama Millimeter Array.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 379 - 381
Copyright
Copyright © Astronomical Society of the Pacific 1994

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