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The H i content of star-forming galaxies at z= 0.24
Authors:Philip Lah  Jayaram N Chengalur  Frank H Briggs  Matthew Colless  Roberto De Propris  Michael B Pracy  W J G de Blok  Shinobu S Fujita  Masaru Ajiki  Yasuhiro Shioya  Tohru Nagao  Takashi Murayama  Yoshiaki Taniguchi  Masafumi Yagi  Sadanori Okamura
Institution:Research School of Astronomy &Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia;National Centre for Radio Astrophysics, Post Bag 3, Ganeshkhind, Pune 411 007, India;Australian Telescope National Facility, Epping, NSW 2111, Australia;Anglo-Australian Observatory, PO Box 296, Epping, NSW 2111, Australia;Cerro Tololo Inter-American Observatory, Casilla 603, La Serena, Chile;Astronomical Institute, Graduate School of Science, Tohoku University, Aramaki, Aoba, Sendai 980-8578, Japan;Physics Department, Graduate School of Science and Engineering, Ehime University, 2-5 Bunkyo-cho, Matsuyama 790-8577, Japan;National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;Department of Astronomy and Research Centre for the Early Universe, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
Abstract:
Keywords:galaxies: evolution  galaxies: ISM  radio continuum: galaxies  radio lines: galaxies
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