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Dark Matter in the Milky Way

Published online by Cambridge University Press:  07 August 2017

Konrad Kuijken*
Affiliation:
Kapteyn Astronomical Instituut, P.O. Box 800, 9700 AV, Groningen, the Netherlands Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge MA 02138, USA ([email protected])

Extract

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If the Newtonian inverse-square law is an appropriate description of gravity, then disk galaxies, and the Milky Way in particular, contain large amounts of dark matter: in general, the observed shapes of rotation curves do not correspond to the gravitational potential of the observed stars and gas. The nature of this dark matter is still a topic of debate, the outcome of which will have important consequences for our ideas of how galaxies and larger structures in the universe formed.

Type
Session 5: Dark Matter in Galaxies
Copyright
Copyright © Kluwer 1995 

References

Alcock, C. et al., 1993, Nature 365, 621 Google Scholar
Aubourg, E. et al., 1993, Nature 365, 623 Google Scholar
Bahcall, J.N., 1984a, Ap. J. 276, 156 Google Scholar
Bahcall, J.N., 1984b, Ap. J. 276, 169 Google Scholar
Bahcall, J.N., 1984c, Ap. J. 287, 926 Google Scholar
Bahcall, J.N., Flynn, C. and Gould, A., 1992, Ap. J. 389, 234 Google Scholar
Bessel, M.S. and Stringfellow, G.S., 1993, Ann. Rev. Astron. Astroph. 31, 433 Google Scholar
Bienaymé, O., Robin, A.C. and Crézé, , 1987, A. & A. 180, 94 Google Scholar
Comeron, F., Torra, J., Gomez, A. E., 1992, Astroph & Spa. Sci. 187, 187 Google Scholar
Fich, M. and Tremaine, S., 1991, Ann. Rev. Astron. Astroph. 29, 409 Google Scholar
Flynn, C. and Fuchs, B., 1994, M. N. R. A. S., in press Google Scholar
Fuchs, B. and Wielen, R., 1993, Back to the Galaxy, eds. Holt, S. S. and Verter, F., p. 580 Gould, A., 1990, M. N. R. A. S. 244, 25 Google Scholar
Gould, A., 1994, preprint Google Scholar
Hartkopf, W.I. and Yoss, K.M., 1982, A. J. 87, 1679 Google Scholar
Hill, G., Hilditch, R.W. and Barnes, J.V., 1979, M. N. R. A. S. 186, 813 Google Scholar
Kapteyn, J.C., 1922, Ap. J. 55, 302 Google Scholar
Kent, S.M., 1992, Ap. J. 387, 181 Google Scholar
Kiraga, M. and Paczyński, B., 1994, Ap. J. 430, L101 Google Scholar
Kuijken, K., 1991, Ap. J. 372, 125 CrossRefGoogle Scholar
Kuijken, K. and Gilmore, G., 1989a, M. N. R. A. S. 239, 605 Google Scholar
Kuijken, K. and Gilmore, G., 1989b, M. N. R. A. S. 239, 650 Google Scholar
Kuijken, K. and Gilmore, G., 1991, Ap. J. 367, L9 Google Scholar
Merrifield, M.R., 1993, Back to the Galaxy, eds. Holt, S.S. and Verter, F., p.437 Google Scholar
Oort, J.H., 1932, Bull. Astron. Neth. 6, 249 Google Scholar
Paczyński, B., 1986, Ap. J. 304, 1 Google Scholar
Richstone, D., Gould, A., Guhathakurta, P. and Flynn, C., 1992, Ap. J. 388, 354 Google Scholar
Richer, H.B. and Fahlman, G.G., 1992, Nature 358, 383 Google Scholar
Schechter, P. 1993, Back to the Galaxy, eds. Holt, S.S. and Verter, F., p. 571 Google Scholar
Udalski, A., et al., 1994, Acta Astronomica 44, 165.Google Scholar
Wood, M.A., 1992, Ap. J. 386, 539 Google Scholar
Yuan, J.W., 1989, A. & A. 224, 108 Google Scholar