Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-26T03:33:00.306Z Has data issue: false hasContentIssue false

Where Does the Galaxy End?

Published online by Cambridge University Press:  25 May 2016

F.D.A. Hartwick*
Affiliation:
Department of Physics and Astronomy, University of Victoria, Victoria, B.C., Canada, V8W 3P6

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.

The spatial distribution of the outlying satellites of the Galaxy has been determined by fitting a three dimensional surface to the positions of 10 companion galaxies and 13 distant globular clusters. Both groups show a highly flattened distribution whose minor axes are aligned to within ∼ 5°. The combined group of 23 objects shows a triaxial distribution with semimajor axis extending ∼ 400 kpc. The minor axis is inclined at ∼ 76° to the Galactic poles. There is a suggestion of a nested hierarchy consisting of satellite galaxies, globular clusters, and distant halo field stars, in order of decreasing spatial extension.

Type
Chapter 8: How do we put it together?
Copyright
Copyright © Kluwer 1996 

References

Arnold, R., Gilmore, G. (1992), Mon. Not. R. astr. Soc. , 257, 225.Google Scholar
Bahcall, J., Flynn, C., Gould, A., Kirhakos, S. (1994), Astrophys. J. , in press.Google Scholar
Binney, J.J. (1992), Ann. Rev. Astron. Astrophys. , 30, 51.Google Scholar
Bothun, G., Elias, J.H., MacAlpine, G. et al. (1991), Astron. J. , 101, 2220.Google Scholar
Burton, W.B. (1992), in The Galactic Interstellar Medium , ed. Pfenniger, D. & Bartholdi, P. (New York: Springer-Verlag), 134.Google Scholar
Ciardullo, R., Jacoby, G., Bond, H. (1989), Astron. J. , 98, 1648.CrossRefGoogle Scholar
Dubinski, J. (1994), submitted to Astrophys. J. Google Scholar
Dubinski, J., Carlberg, R.G. (1991), Astrophys. J. , 378, 496.Google Scholar
Frenk, C.S., White, S.D.M., Davis, M., Efstathiou, G. (1988), Astrophys. J. , 327, 507.Google Scholar
Freudenreich, H.T., Berriman, G.B., Dwek, E. et al. (1994), Astrophys. J. Lett , 429, L69.Google Scholar
Green, P.J., Margon, B., and Erson, S.F., Cook, K.H. (1994), Astrophys. J. , in press.Google Scholar
Hawkins, M.R.S. (1984), Mon. Not. R. astr. Soc. , 206, 433.Google Scholar
Ibata, R.A., Gilmore, G., Irwin, M.J. (1994), Nature , 370, 194.CrossRefGoogle Scholar
Kapteyn, J.C. (1922), Astrophys. J. , 55, 302.Google Scholar
Katz, N. (1992), Astrophys. J. , 391, 502.Google Scholar
Katz, N., Gunn, J.E. (1991), Astrophys. J. , 377, 365.Google Scholar
Kunkel, W.E. (1979), Astrophys. J. , 228, 718.Google Scholar
Kunkel, W.E., Demers, S. (1976), R. Greenwich Obs. Bull. , No. 182, 241.Google Scholar
Lanzetta, K.M., Bowen, D.V., Tytler, D., Webb, J.K. (1994), Astrophys. J. , in press.Google Scholar
Lynden-Bell, D. (1976), R. Greenwich Obs. Bull. , No. 182, 235.Google Scholar
Lynden-Bell, D. (1982), Observatory , 102, 202.Google Scholar
Majewski, S.R. (1994), Astrophys. J. Lett , 431, L17.Google Scholar
Norris, J.E., Hawkins, M.R.S. (1991), Astrophys. J. , 380, 104.Google Scholar
Plaskett, J.S., Pearce, J.A. (1935), Publ. Dom. Astrophys. Obs. , 5, 239.Google Scholar
Rees, M. (1986), Mon. Not. R. astr. Soc. , 218, 25P.CrossRefGoogle Scholar
Richer, H.B., Fahlman, G.G. (1992), Nature , 358, 383.Google Scholar
Richstone, D., Gould, A., Guhathakurta, P., Flynn, C. (1992), Astrophys. J. , 388, 354.Google Scholar
Saha, A. (1984), Astrophys. J. , 283, 580.Google Scholar
Shapley, H. (1918), Astrophys. J. , 48, 154.Google Scholar
Sommer-Larsen, J., Christensen, P.R. (1986), Mon. Not. R. astr. Soc. , 219, 537.Google Scholar
Sommer-Larsen, J., Christensen, P.R., Carter, D. (1989), Mon Not. R. astr. Soc. , 238, 225.Google Scholar
Tello, C. (1994), Astron. J. , 107, 1381.Google Scholar
van den Bergh, S. (1994), Astron. J. , 107, 1328.Google Scholar
Warren, M.S., Quinn, P.J., Salmon, J.K., Zurek, W.H. (1992), Astrophys. J. , 399, 405.Google Scholar