Gemini Near Infrared Spectrograph Observations of a Red Star Forming Galaxy at z=2.225: Evidence for Shock-Ionization due to a Galactic Wind

Details Gemini Near Infrared Spectrograph Observations of a Red Star Forming Galaxy at z=2.225: Evidence for Shock-Ionization due to a Galactic Wind Gemini Near Infrared Spectrograph Observations of a Red Star Forming Galaxy at z=2.225: Evidence for Shock-Ionization due to a Galactic Wind

2005-02-03

arxiv.org/abs/astro-ph/0502082v1

Astrophys.J. 622 (2005) L13-L16

Astronomy and Astrophysics

Astrophysics

Accepted for publication in the Astrophysical Journal Letters. 4 pages, 3 figures

Scientific paper

10.1086/429376

Recent studies have shown that K-luminous galaxies at 22 galaxies should be regarded with caution, especially since the existence of strong galactic winds in these objects is well established. [ABRIDGED]

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