English

A 3D Optical Spectroscopy Study of Low Surface Brightness Galaxies

Astrophysics 2007-05-23 v1

Abstract

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.

Cite

@article{arxiv.astro-ph/0309596,
  title  = {A 3D Optical Spectroscopy Study of Low Surface Brightness Galaxies},
  author = {L. Chemin and P. Amram and C. Carignan and C. Balkowski and W. van Driel and V. Cayatte and O. Hernandez and J. Boulesteix and M. Marcelin},
  journal= {arXiv preprint arXiv:astro-ph/0309596},
  year   = {2007}
}

Comments

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

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