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Spiral Galaxy in 3D as Seen with SpIOMM

Published online by Cambridge University Press:  09 February 2015

Laurie Rousseau-Nepton ,
Carmelle Robert  and
Laurent Drissen
Laurie Rousseau-Nepton
Affiliation:
Université Laval & Centre de Recherche en Astrophysique du Québec, Québec, Canada
Carmelle Robert
Affiliation:
Université Laval & Centre de Recherche en Astrophysique du Québec, Québec, Canada
Laurent Drissen
Affiliation:
Université Laval & Centre de Recherche en Astrophysique du Québec, Québec, Canada
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Abstract

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Using the imaging Fourier transform spectrograph (FTS) SpIOMM we study 7 nearby spiral galaxies. The large database of spectra obtained around Hα and Hβ is ideal to study the star forming regions and warm ionized medium (WIM) with a high spatial resolution (∼ 50-150 pc).

Keywords

galaxies: nearby spiralgalaxies: evolution - galaxies: star formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 340
Copyright
Copyright © International Astronomical Union 2015 

References

Blanc, G. A., et al. 2009, ApJ, 704, 842Google Scholar
Haffner, L. M., et al. 1999, ApJ, 523, 223Google Scholar