Supersonic Motions in Giant H II Regions: Handling 3D Data with Matador
Bidimensional spectroscopy with good spatial and spectral resolution, sampling a particular emission line over the whole emitting area, is shown here to be the most suitable observational technique for understanding the kinematics of giant extragalactic H II regions (GEHRs). The TAURUS II Fabry-Perot spectrograph is an excellent instrument for this
Munoz-Tunon, C. et al.
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1995