The Morphology of Nearby Low Surface Brightness Galaxies

Details The Morphology of Nearby Low Surface Brightness Galaxies The Morphology of Nearby Low Surface Brightness Galaxies

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap%26ss.269..101d&link_type=abstract

Astrophysics and Space Science, v. 269/270, p. 101-108 (1999).

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

It is commonly assumed that low surface brightness (LSB) galaxies are dormant and quiescent systems. These conclusions are however based on observations of a large number of distant LSB galaxies. Here we show some first results of a study of very nearby galaxies, which suggest that the featureless systems observed at large distances resolve into complex and chaotic systems. We also present new data on NGC 6822, a dwarf galaxy in our Local Group, and argue that this object would be classified as a LSB galaxy if it were at a larger distance. It thus puts us in the unique position of being able to study a LSB galaxy at very high resolution, enabling us to get a better picture of the interaction between ISM, stars and dark matter in low density galaxies.

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