University of Hertfordshire

HI properties of Low Surface Brightness dwarf and blue compact dwarf galaxies

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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Original languageEnglish
Title of host publicationIn: Procs of Low Surface Brightness Universe, IAU Colloquium 171, ASP Conference Series 170
PublisherAstronomical Society of the Pacific
Pages337-339
ISBN (Print)1-886733-92-9
Publication statusPublished - 1999

Abstract

We present high resolution (~15") VLA HI observations of one LSB dwarf galaxy and 5 Blue Compact Dwarfs. Previous works have emphasized the difference in the peak column density of the HI between the two types of galaxy. However, the peak column density is typically only a factor of 2-4 greater in BCDs than in LSB dwarfs, suggesting that the difference between the two is one of degree, not quality. The HI morphologies of the two types are often quite similar.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific

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