Thèse--Lettres. / Bibliogr. p. 316-355.

Thesis (doctoral) - Harvard Law School, Cambridge, Mass., 2005. / Includes bibliographical references.

Thesis (PH. D.)--Cornell University. / Reprinted from the American Journal of Mathematics, vol. XXIX, no. 4.

Thesis (Ph. D.)--University of Chicago, Dept. of Physics, August 1999. / Includes bibliographical references. Also available on the Internet.

Thesis (Ph. D.)--Public Policy, Georgia Institute of Technology, 2006. / Gregory B. Lewis, Committee Chair ; Douglas Noonan, Committee Member ; Sally Wallace, Committee Member ; Michael Rushton, Committee Member ; Bruce Seaman, Committee Member.

Thesis--University of Florida. / Description based on print version record. Typescript. Vita. Includes bibliographical references (vol. 2, leaves 780-785).

Thesis (Ph. D.)--University of Texas at Austin, 1999. / Vita. Includes bibliographical references (leaves 178-184). Available also in a digital version from Dissertation Abstracts.

Boston University. University Professors Program Senior theses. / PLEASE NOTE: Boston University Libraries did not receive an Authorization To Manage form for this thesis. It is therefore not openly accessible, though it may be available by request. If you are the author or principal advisor of this work and would like to request open access for it, please contact us at open-help@bu.edu. Thank you. / 2031-01-02

Amergin and Cessair is a musical setting of the text "Amergin and Cessair: A Battle of Poetic Incantation" by Michael Meade and Erica Helm Meade. The music takes the form of a dramatic "duet," scored for double choir and chamber orchestra. It depicts an exchange of self-exalting verses proclaimed by the two demigods Amegin and Cessair. Cessair--an early inhabitant of Ireland--uses her verses to churn the sea and fend off ship-borne Amergin, who in turn calms the sea with his verses. Musically, the two characters are distinguished by their own unique melodic motives, harmonic sonorities, and instrumentations. The drama of the battle unfolds over the course of the fifteen-minute work, and ultimately Amergin is the victorious one. Overall, the work expresses the pride, determination, and intense emotionality of the two characters objectively, without taking the side of either one, and it is an allegory for cultural conflict.

The application of the discrete Fourier transform to the determination of the frequency content of unevenly-sampled astronomical time series is discussed, and an interactive computer package which incorporates a variety of power-spectrum and time-domain techniques is described. A frequency analysis of the light curves of two hot, extreme helium stars, BD-9°4395 and HD160641, shows that their photometric variability is caused by non-radial pulsation. Spectroscopic evidence in support of non-uniform mass loss is presented for BD-9°4395. Spectroscopic and photometric observations of two early-type eclipsing binary systems, AL Sculptoris and DM Persei, have been analysed to yield their absolute dimensions. AL Scl is found to be a detached system in which both components rotate faster than synchronism. The origin of distortions in its light curve is unclear. DH Per is shown to be part of a triple system in which the third component is most probably a late-B star in a 98-day orbit with a semi-major axis of 0.9 A.U. The binary system is confirmed to be semi-detached and to have evolved through a phase of rapid mass transfer. DH Per joins a small group of massive, semi-detached systems whose characteristics differ significantly from the classical Algols, and which may result from case-A, mass-transfer processes. Spectroscopic and photometric observations of the F4V star HD123058 do not support the hypothesis that it is a binary system. Broad lines in its spectrum are attributed to a somewhat enhanced rotation rate, and the star is shown to be essentially unevolved. The derivation of the equation of condition in Sterne's rigorous method for the analysis of the spectroscopic elements of binary systems, and its modification for incorporating observed times of minimum light into the adjustment of the elements, are outlined. A computer code for the determination of orbital elements according to this scheme is described.