The H i content of star-forming galaxies at z = 0.24

Monthly Notices of the Royal Astronomical Society

Volumn 376, Issue 3, 2007, Pages 1357-1366

  Lah, Philip ^a   Chengalur, Jayaram N ^b   Briggs, Frank H ^a,c   Colless, Matthew ^d   De Propris, Roberto ^e   Pracy, Michael B ^a   De Blok W J G ^a   Fujita, Shinobu S ^f   Ajiki, Masaru ^f   Shioya, Yasuhiro ^g   Nagao, Tohru ^h   Murayama, Takashi ^f   Taniguchi, Yoshiaki ^g   Yagi, Masafumi ^h   Okamura, Sadanori ⁱ  

^a AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^b NATIONAL CENTRE FOR RADIO ASTROPHYSICS   (India)

^c CSIRO   (Australia)

^d ANGLO AUSTRALIAN OBSERVATORY   (Australia)

^e CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

^f TOHOKU UNIVERSITY   (Japan)

^g EHIME UNIVERSITY   (Japan)

^h NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

ⁱ UNIVERSITY OF TOKYO   (Japan)

Author keywords

Galaxies: evolution; Galaxies: ISM; Radio continuum: galaxies; Radio lines: galaxies

Indexed keywords

COSMOLOGY; DENSITY OF GASES; LUMINANCE; RADIO ASTRONOMY; STARS;

ATOMIC HYDROGEN; GALAXIES: ISM; GALAXY EVOLUTION; GAS CONTENT; GIANT METREWAVE RADIO TELESCOPES; HYDROGEN GAS; RADIO CONTINUUM: GALAXIES; RADIO LINES:GALAXIES; STAR FORMATION RATES; STAR FORMING GALAXY;

GALAXIES;

EID: 34147131320     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11540.x     Document Type: Article

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