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Models of the mass distribution of the Galaxy

Published online by Cambridge University Press:  04 August 2017

Maarten Schmidt*
Affiliation:
California Institute of Technology Pasadena, California, U.S.A.

Extract

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Mass models of the Galaxy play an important role in studies of the structure of the Galaxy. The various populations or components combine to yield a gravitational field that produces the observed rotation curve. For the spheroid and disk this requirement can be used to set limits on some of their properties. The properties of the dark corona are entirely defined this way.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Copyright
Copyright © Reidel 1985 

References

Bahcall, J.N., Schmidt, M., and Soneira, R.M.: 1982, Astrophys. J. (Letters), 258, L23 Google Scholar
Bahcall, J.N., Schmidt, M., and Soneira, R.M.: 1983, Astrophys. J. 265, 730 CrossRefGoogle Scholar
Caldwell, J.A.R., and Ostriker, J.P.: 1981, Astrophys. J. 251, 61 CrossRefGoogle Scholar
Clutton-Brock, M., Innanen, K.A., and Papp, K.A.: 1977, Astrophys. Space Sci. 47, 299 Google Scholar
de Vaucouleurs, G., and Pence, W.D.: 1978, Astrophys. J. 83, 1163 Google Scholar
Einasto, J.: 1979, in IAU Symposium 84, The Large Scale Characteristics of the Galaxy, ed. Burton, W.B. (Dordrecht: Reidel), p. 451 Google Scholar
Freeman, K.C.: 1970, Astrophys. J. 160, 811 Google Scholar
Harris, W.E.: 1976, Astron. J. 81, 1095 Google Scholar
Isaacman, R., and Oort, M.J.A.: 1981, Astron. Astrophys. 102, 347 Google Scholar
Knapp, G.R.: 1980, private communication Google Scholar
Krumm, N., and Salpeter, E.E.: 1979, Astron. J. 84, 1138 Google Scholar
Miyamoto, M., Satoh, C., and Ohashi, M.: 1980, Astron. Astrophys. 90, 215 Google Scholar
Oort, J.H.: 1960, Bull. Astron. Instit. Netherlands 15, 45 Google Scholar
Oort, J.H., and Plaut, L.: 1975, Astron. Astrophys. 41, 71 Google Scholar
Richstone, D.O., and Graham, F.G.: 1981, Astrophys. J. 248, 516 Google Scholar
Rohlfs, K., and Kreitschmann, J.: 1981, Astrophys. Space Sci. 79, 289 Google Scholar
Rubin, V.C., Ford, W.K., and Thonnard, N.: 1980, Astrophys. J. 238, 471 Google Scholar
Rubin, V.C., Ford, W.K., Thonnard, N., and Burstein, D.: 1982, Astrophys. J. 261, 439 Google Scholar
Schmidt, M.: 1965, in Galactic Structure, ed. Blaauw, A. and Schmidt, M. (Chicago: University of Chicago Press), p. 513 Google Scholar
Schmidt, M.: 1975, Astrophys. J. 202, 22 Google Scholar
Sinha, R.P.: 1978, Astron. Astrophys. 69, 227 Google Scholar
van der Kruit, P.C., and Searle, L.: 1982, Astron. Astrophys. 110, 61 Google Scholar