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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
Affiliation: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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