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References
- 1
- Brookshaw, L., 1985, Proc. Astr. Soc. Australia, 6, 207.
- 2
- Brookshaw, L., 1986, The Stability of Binary Systems and
Rotating Stars, Ph.D. Thesis,
Monash University, Australia.
- 3
- Campbell, P.M., 1988, Some New Algorithms for Boundary
Value Problems in SPH,
DNA-TR-88-286, Mission Research Corp.,
Albequerque.
- 4
- Lorimer, G., 1982, The Stability of Rotating Stars,
Ph.D. Thesis, Monash University, Australia.
- 5
- Lucy, L.B., 1977, Astron. J., 82, 1013.
- 6
- Monaghan, J.J., 1985a, Private Communication.
- 7
- Monaghan, J.J., 1985b, Computer Physics Reports, 3, 71.
- 8
- Monaghan, J.J., 1992, Annu. Rev. Astron. Astrophys., 30, 543.
- 9
- Pongracic, H., 1988, Numerical Modelling of Large Body
Impacts, Ph.D. Thesis, Monash University, Australia.
- 10
- Schwarzschild, M., 1958, Structure and Evolution of the Stars,
Dover Publications, New York.
Leigh Brookshaw
Tue Jun 6 09:55:47 PDT 1995