Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-24T13:28:51.054Z Has data issue: false hasContentIssue false
  • English
  • Français

The Structure of the Superthin Spiral Galaxy UGC7321

Published online by Cambridge University Press:  12 April 2016

L.D. Matthews ,
J.S. Gallagher  and
W. van Driel
L.D. Matthews
Affiliation:
NRAO, Charlottesville, VA, USA
J.S. Gallagher
Affiliation:
University of Wisconsin, Madison, WI, USA
W. van Driel
Affiliation:
Unité Scientifique Nançay, Observatoire de Paris, France

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

UGC 7321 is an edge-on low surface brightness (LSB) spiral galaxy with a number of extraordinary properties. Its vertical scale height (~70 pc) is one of the smallest ever measured for a galaxy disk. Its disk also exhibits strong vertical and radial color gradients. UGC 7321 appears to be an extremely unevolved galaxy in both a dynamical and in a star-formation sense.

Type
Properties of Low Surface Brightness galaxies
Information
International Astronomical Union Colloquium , Volume 171: The Low Surface Brightness Universe , 1999 , pp. 207 - 209
Copyright
Copyright © Astronomical Society of the Pacific 1999

References

Matthews, L.D. 1998, Ph.D. Thesis, State University of New York at Stony Brook Google Scholar
Tully, R.B., Shaya, E.J., & Pierce, M.J. 1992, ApJS, 80, 479 CrossRefGoogle Scholar
van der Kruit, P.C. & Searle, L. 1981, A&A, 95, 105 Google Scholar