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Approximate third integrals for axisymmetric potentials using local Stackel fits.

Veronique De Bruyne UGent, Francine Leeuwin and Herwig Dejonghe UGent (2000) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 311(2). p.297-306
Please use this url to cite or link to this publication:
author
organization
year
type
journalArticle
publication status
published
subject
journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Mon. Not. Roy. Astron. Soc.
volume
311
issue
2
pages
297-306 pages
Web of Science type
Article
Web of Science id
000084670100006
ISSN
0035-8711
language
English
UGent publication?
yes
classification
A1
id
123691
handle
http://hdl.handle.net/1854/LU-123691
date created
2004-01-14 13:36:00
date last changed
2008-02-22 22:45:19
@article{123691,
  author       = {De Bruyne, Veronique and Leeuwin, Francine and Dejonghe, Herwig},
  issn         = {0035-8711},
  journal      = {MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY},
  language     = {eng},
  number       = {2},
  pages        = {297--306},
  title        = {Approximate third integrals for axisymmetric potentials using local Stackel fits.},
  volume       = {311},
  year         = {2000},
}

Chicago
De Bruyne, Veronique, Francine Leeuwin, and Herwig Dejonghe. 2000. “Approximate Third Integrals for Axisymmetric Potentials Using Local Stackel Fits.” Monthly Notices of the Royal Astronomical Society 311 (2): 297–306.
APA
De Bruyne, V., Leeuwin, F., & Dejonghe, H. (2000). Approximate third integrals for axisymmetric potentials using local Stackel fits. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 311(2), 297–306.
Vancouver
1.
De Bruyne V, Leeuwin F, Dejonghe H. Approximate third integrals for axisymmetric potentials using local Stackel fits. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2000;311(2):297–306.
MLA
De Bruyne, Veronique, Francine Leeuwin, and Herwig Dejonghe. “Approximate Third Integrals for Axisymmetric Potentials Using Local Stackel Fits.” MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 311.2 (2000): 297–306. Print.