D. References

In addition to a standard bibliography which contains references to published research that has been discussed in the body of this proposal, in this section we also include an itemized list (Jnn) of 18 articles and dissertations that have acknowledged the PI's support over the past four years and an itemized list (Mnn) of 18 Quicktime movies that have been produced by the PI's researh group from fluid dynamic simulations that are relevant to the research discussed in the body of this proposal.

Bibliography

Digital Animation Sequences (Quicktime Movies)

Title and URL References
M1.  Stable, Common-Envelope, Equal-Mass Polytropic Binary [J2, J7]
http://www.phys.lsu.edu/astro/movie_captions/equalmass.binary.html
M2.  Merger of Close, Equal-Mass Polytropic Binary [J2, J7, J14]
http://www.phys.lsu.edu/astro/movie_captions/equalmass.binary.html
M3.  Andalib's Prograde Flow [J11]
http://www.phys.lsu.edu/astro/movie_captions/Andalib.html
M4.  Andalib's Common-Envelope Binary Flow [J11]
http://www.phys.lsu.edu/astro/barmode/movies/bin_sa.mov
M5.  Fluid Flow in Four of Andalib's Nonaxisymmetric Disk Models [J11, J13]
http://www.phys.lsu.edu/astro/movie_captions/Andalib.html
M6.  Bar-mode Instability in Rapidly Rotating, n=3/2 (n'=0) Polytrope [J13, J14, J16, J18]
http://www.phys.lsu.edu/astro/movie_captions/two_armed_spiral.html
M7.  Bar-mode Instability in n=3/2 Polytrope with Uniform Vortensity [J16, J18]
http://www.phys.lsu.edu/astro/movie_captions/two_armed_spiral.html
[NOTE: In the following movie titles, C.A.R.E. means Compressible Analog of a Riemann Ellipsoid]
M8.  C.A.R.E. (Model A) Steady-State, 3-D Density Structure [J13, J16, J18]
http://www.phys.lsu.edu/astro/movie_captions/cares.html
M9.  C.A.R.E. (Model A) Equatorial Flow [J13, J16, J18]
http://www.phys.lsu.edu/astro/movie_captions/cares.html
M10.  C.A.R.E. (Model A) Meridional Flow [J13, J16, J18]
http://www.phys.lsu.edu/astro/movie_captions/cares.html
M11.  C.A.R.E. (Model B) Steady-State, 3-D Density Structure [J16, J18]
http://www.phys.lsu.edu/astro/movie_captions/cares.html
M12.  C.A.R.E. (Model B) Equatorial Flow [J16, J18]
http://www.phys.lsu.edu/astro/movie_captions/cares.html
M13.  Fission Instability [J16]
http://www.phys.lsu.edu/astro/movie_captions/fission.html
M14.  Proto-binary Equatorial Flow [J14, J16]
http://www.phys.lsu.edu/astro/movie_captions/fission.html
M15.  Proto-binary Meridional Flow [J14, J16]
http://www.phys.lsu.edu/astro/movie_captions/fission.html
M16.  Stable, Polytropic Binary with Mass Ratio q = 0.81
http://www.phys.lsu.edu/astro/movie_captions/motl.binary.html
M17.  Mass-Transferring Binary with Mass Ratio q = 0.88 (Stream)
http://www.phys.lsu.edu/astro/movie_captions/motl.binary.html
M18.  Mass-Transferring Binary with Mass Ratio q = 0.88 (Equatorial slice)
http://www.phys.lsu.edu/astro/movie_captions/motl.binary.html