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The Shapes of Dark Halos

Published online by Cambridge University Press:  25 May 2016

Hans-Walter Rix
Hans-Walter Rix*
Affiliation:
Institute for Advanced Study, Princeton, NJ 08540, USA Max-Planck-Institut für Astrophysik, 85740 Garching, Germany

Extract

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Galactic and extragalactic astronomers often mean different things by “halo” the former mean the spheroidal distribution of metal poor stars around the Milky Way (MW), the latter mean the massive, dark component providing the large dynamically inferred mass in and around galaxies. This review will focus on massive, dark halos. Despite the title of this conference, we cannot restrict our attention to the shape of the MW halo: very little would be to say. We must turn to cosmological simulations and to observations of external disk galaxies in the hope of deriving a representative picture.

Type
Chapter 1: Are the Disk and Halo Axisymmetric?
Information
Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 23 - 30
Copyright
Copyright © Kluwer 1996 

References

Amendt, P. and Cuddeford, P., 1994, preprint. Google Scholar
Binney, J., May, A. and Ostriker, J. P., 1987, MNRAS, 226, 149.Google Scholar
Binney, J. and de Vaucouleurs, G., 1981, MNRAS, 194, 679.CrossRefGoogle Scholar
Buote, D. and Canizares, C., 1992 ApJ, 400, 385.CrossRefGoogle Scholar
Buote, D. and Canizares, C., 1994 ApJ, 427, 86.CrossRefGoogle Scholar
Dubinski, J. and Carlberg, R., 1991, Ap.J., 369, 13.Google Scholar
Dubinski, J., 1994, preprint. Google Scholar
Dubinski, J. and Kuijken, K., 1994, preprint. Google Scholar
Fasano, G. et al., 1993, MNRAS, 262, 109.Google Scholar
Franx, M. and de Zeeuw, T., 1992, ApJL, 392, 47.CrossRefGoogle Scholar
Franx, M., van Gorkom, J. and de Zeeuw, T., 1994, ApJ, in press. Google Scholar
Hartwick, F. D. A., 1983, MmSocAstIt, 54, 51.Google Scholar
Hawkins, M. R. S., 1984, MNRAS, 206, 433.Google Scholar
Huizinga, J.E. and van Albada, T.S., 1992, MNRAS, 254, 677.Google Scholar
Katz, N., 1991, Ap.J., 368, 325.CrossRefGoogle Scholar
Katz, N. and Gunn, J. E., 1991, Ap.J., 377, 365.Google Scholar
Maloney, P., 1993, ApJ, 414, 41.Google Scholar
Morrison, H., Flynn, C. and Freeman, K., 1990, A.J., 100, 1191.CrossRefGoogle Scholar
Rix, H.-W. and Katz, N., 1991, in Polar Rings and Inclined Disks in Galaxies , Cambridge Univ. Press, Eds: Casertano, S., Sackett, P. and Briggs, F. Google Scholar
Rix, H.-W. and Zaritsky, D. F., 1994, Ap.J. submitted. Google Scholar
Sackett, P. and Sparke, L., 1990, ApJ, 361 408.Google Scholar
Sackett, P., Rix, H.-W., Jarvis, B. and Freeman, K., 1994, Ap.J., in press. Google Scholar
Sommer-Larsen, J. and Zhen, C., 1990, MNRAS, 242, 10.CrossRefGoogle Scholar
Summers, F., 1993, Ph.D. Thesis, Univ. of California, Berkeley.Google Scholar
van der Marel, R. P., 1991, MNRAS, 248, 515.Google Scholar
Warren, M. S., Quinn, P. J., Salmon, J. K. and Zurek, W. H., 1992, Ap.J., 399, 405.Google Scholar
Wyse, R. F. G, and Gilmore, G., 1986, A.J., 91, 855.CrossRefGoogle Scholar