A 3D Optical Spectroscopy Study of Low Surface Brightness Galaxies

Details A 3D Optical Spectroscopy Study of Low Surface Brightness Galaxies A 3D Optical Spectroscopy Study of Low Surface Brightness Galaxies

2003-09-22

arxiv.org/abs/astro-ph/0309596v1

Astronomy and Astrophysics

Astrophysics

2 pages, 4 figures, to be published in "IAU Symposium 220, Dark matter in galaxies", ASP Conf Series

Scientific paper

We present Halpha emission line velocity fields of two Low Surface Brightness
galaxies - UGC 628 and UGC 5005 - obtained using Fabry-Perot interferometry
observations at the Canada-France-Hawaii telescope. Our goal is to study the
dynamics of Low Surface Brightness galaxies.

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