Abstract
We present recent results from the Blind Ultra Deep HI Environmental
Survey (BUDHIES), that has detected over 150 galaxies at z˜ 0.2
with the Westerbork Synthesis Radio Telescope (WSRT). Our
multi-wavelength study is the first where optical properties and HI
content are combined at a redshift where evolutionary effects begin to
show. Our goal is to study the link between the environment, HI content,
morphology, stellar mass and star formation in galaxies at z˜ 0.2,
and the importance of different physical mechanisms in the
transformation of galaxies.
Original language | English |
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Title of host publication | BUDHIES: a Blind Ultra Deep HI Environmental Survey |
Pages | 80-80 |
Volume | 44 |
Publication status | Published - 1-Oct-2014 |
Keywords
- H I gas
- Galaxies