2D kinematics and physical properties of z similar to 3 star-forming galaxies
We present results from a study of the kinematic structure of star-forming galaxies at redshift z ∼ 3 selected in the VIMOS VLT Deep Survey (VVDS), using integral field spectroscopy of rest-frame optical nebular emission lines, in combination with rest-frame UV spectroscopy, ground-based optical/nea...
Päätekijät: | Lemoine-Busserolle, M, Bunker, A, Lamareille, F, Kissler-Patig, M |
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Aineistotyyppi: | Journal article |
Kieli: | English |
Julkaistu: |
2010
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