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Kinematics of Giant Low Surface Brightness Galaxies

Published online by Cambridge University Press:  12 April 2016

T.E. Pickering
T.E. Pickering*
Affiliation:
Kapteyn Institute, Postbus 800, 9700 AV Groningen, The Netherlands

Abstract

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High sensitivity H I observations now exist for six giant low surface brightness (LSB) disk galaxies including the two prototypes, Malin 1 (Bothun et al. 1987; Impey & Bothun 1989) and F568-6 (also known as Malin 2; Bothun et al. 1990). Their H I surface brightnesses are generally low, but proportionally not as low as their optical surface brightnesses. Their total H I masses and radial extents are quite large, however, with MHI ∼ 1010M⊙h−275 and with detectable H I out to 100 kpc h−175 or more in a couple of cases. The rotation curves of these systems rise slowly and are consistent with negligible disk contribution, similar to many previously observed dwarf galaxies. However, the peak rotation velocities of these galaxies are high (>200 km s−1) and infer high dynamical masses. These galaxies provide the some of the first examples of galaxies that are both massive and dark matter dominated.

Type
Properties of Low Surface Brightness galaxies
Information
International Astronomical Union Colloquium , Volume 171: The Low Surface Brightness Universe , 1999 , pp. 214 - 220
Copyright
Copyright © Astronomical Society of the Pacific 1999

References

Begeman, K.G. 1989, A&A, 223, 47 Google Scholar
Broeils, A.H. 1992, Ph.D. thesis, University of Groningen Google Scholar
de Blok, W.J.G., McGaugh, S.S., & van der Hulst, J.M. 1996, MNRAS, 283, 18 CrossRefGoogle Scholar
de Blok, W.J.G., & McGaugh, S.S. 1997, MNRAS, 290, 533 CrossRefGoogle Scholar
Bothun, G.D., Impey, C.D., Malin, D.F., & Mould, J.R. 1987, AJ, 94, 23 CrossRefGoogle Scholar
Bothun, G.D., Schombert, J.M., Impey, C.D., & Schneider, S.E. 1990, ApJ, 360, 427 CrossRefGoogle Scholar
Casertano, S., & van Gorkom, J.H. 1991, AJ, 101, 1231 CrossRefGoogle Scholar
Disney, M.J. 1976, Nature, 263, 573 CrossRefGoogle Scholar
Impey, C.D., & Bothun, G.D. 1989, ApJ, 341, 89 CrossRefGoogle Scholar
Impey, C.D., Sprayberry, D., Irwin, M.J., & Bothun, G.D. 1996, ApJS, 105, 209 CrossRefGoogle Scholar
Kennicutt, R.C. 1989, ApJ, 344, 685 CrossRefGoogle Scholar
Knezek, P.M. 1993, Ph.D. thesis, University of Massachusetts Google Scholar
McGaugh, S.S. 1992, Ph.D. thesis, University of Michigan Google Scholar
Navarro, J.F., Frenk, C.S., & White, S.D.M. 1996, ApJ, 462, 563 CrossRefGoogle Scholar
Navarro, J.F., Frenk, C.S., & White, S.D.M. 1997, ApJ, 490, 493 CrossRefGoogle Scholar
Pickering, T.E., Impey, C.D., van Gorkom, J.H., & Bothun, G.D. 1996, AJ, 114, 1858 CrossRefGoogle Scholar
Pickering, T.E. 1998, Ph.D. thesis, University of Arizona Google Scholar
Quillen, A., & Pickering, T.E. 1997, AJ, 113, 2075 CrossRefGoogle Scholar
Schombert, J.S., & Bothun, G.D. 1988, AJ, 95, 1389 CrossRefGoogle Scholar
Sprayberry, D., Impey, C.D., Irwin, M.J., McMahon, R.G., & Bothun, G.D. 1993, ApJ, 417, 114 CrossRefGoogle Scholar
Sprayberry, D., Impey, C.D., Bothun, G.D., & Irwin, M.J. 1995a, AJ, 109, 558 CrossRefGoogle Scholar
Sprayberry, D., Bernstein, G.M., Impey, C.D., & Bothun, G.D. 1995b, ApJ, 438, 72 CrossRefGoogle Scholar
van der Hulst, J.M., Skillman, E.D., Smith, T.R., Bothun, G.D., McGaugh, S.S., & de Blok, W.J.G. 1993, AJ, 106, 548 CrossRefGoogle Scholar
Walsh, W., Staveley-Smith, L., & Oosterloo, T. 1997, AJ, 113, 1591 CrossRefGoogle Scholar
Zwaan, M.A., van der Hulst, J.M., de Blok, W.J.G., & McGaugh, S.S. 1995, MNRAS, 273, L35 CrossRefGoogle Scholar