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HI Properties of LSB Dwarf and Blue Compact Dwarf Galaxies

Published online by Cambridge University Press:  12 April 2016

C.L. Taylor ,
E. Brinks  and
E.D. Skillman
C.L. Taylor
Affiliation:
Astronomisches Institut, Ruhr-Universität Bochum, Germany
E. Brinks
Affiliation:
Depto. de Astronomía, Universidad de Guanajuato, Mexico
E.D. Skillman
Affiliation:
Dept. of Astronomy, University of Minnesota, Minneapolis, USA

Abstract

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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.

Type
HI and QSO absorption lines
Information
International Astronomical Union Colloquium , Volume 171: The Low Surface Brightness Universe , 1999 , pp. 337 - 339
Copyright
Copyright © Astronomical Society of the Pacific 1999

References

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