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F(E,Lz) for Kent's Model of the Galactic Bulge?

Published online by Cambridge University Press:  25 May 2016

Walter Dehnen
Walter Dehnen*
Affiliation:
Theoretical Physics Oxford, OX1 3NP United Kingdom

Abstract

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Using the Richardson-Lucy algorithm the two-integral distribution function (2I-DF) f(E,Lz ) for Kent's (1992) Bulge model has been constructed. It turns out to be negative (and hence unphysical) at Lz ≈ Lc. The physical reason for this result and its implications are discussed.

Type
Chapter 4: Is there a Consistent Picture of the Inner kpc of the Milky Way?
Information
Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 351 - 352
Copyright
Copyright © Kluwer 1996 

References

Dehnen, W., 1994, MNRAS, submitted Google Scholar
Evans, N.W., 1994, MNRAS 267, 333 Google Scholar
Hunter, C., Qian, E., 1993, MNRAS 262, 401 Google Scholar
Kent, S.M., 1992, ApJ 387, 181 Google Scholar
Kuijken, K., 1994, preprint Google Scholar
Lucy, L.B., 1974, AJ 79, 745 Google Scholar
Richardson, W.H., 1972, J. Opt. Soc. Am. 62, 55 Google Scholar