The Cult of 'Maria Regina' in Early Medieval Rome

This paper examines the importance of the cult of Mary to religious practice in early medieval Rome, with a particular focus on the manifestations of devotion to Mary in the decoration of churches such as S. Maria Antiqua and San Clemente.

Melancholy and the Early Modern University

Critics have observed that in early Stuart England, the broad, socially significant concept of melancholy was recoded as a specifically medical phenomenon—a disease rather than a fashion. This recoding made melancholy seem less a social attitude than a private ailment. However, I argue that at the Stuart universities, this recoded melancholy became a covert expression of the disillusionment, disappointment, and frustration produced by pressures there—the overcrowding and competition which left many men “disappointed” in preferment, alongside James I’s unprecedented royal involvement in the universities. My argument has implications for Jürgen Habermas’s account of the emergence of the public sphere, which he claims did not occur until the eighteenth-century. I argue that although the university was increasingly subordinated to the crown’s authority, a lingering sense of autonomy persisted there, a residue of the medieval university’s relative autonomy from the crown; politicized by the encroaching Stuart presence, an alienated community at the university formed a kind of public in private from authority within that authority’s midst. The audience for the printed book, a sphere apart from court or university, represented a forum in which the publicity at the universities could be consolidated, especially in seemingly “private” literary forms such as the treatise on melancholy. I argue that Robert Burton’s exaggerated performance of melancholy in The Anatomy of Melancholy, which gains him license to say almost anything, resembles the performed melancholy that the student-prince Hamlet uses to frustrate his uncle’s attempts to surveil him. After tracing melancholy’s evolving literary function through Hamlet, I go on to discuss James’s interventions into the universities. I conclude by considering two printed (and widely circulated) books by university men: the aforementioned The Anatomy of Melancholy by Burton, an Oxford cleric, and The Temple by George Herbert, who left a career as Cambridge’s public orator to become a country parson. I examine how each of these books uses the affective pattern of courtly-scholarly disappointment—transumed by Burton as melancholy, and by Herbert as holy affliction—to develop an empathic form of publicity among its readership which is in tacit opposition to the Stuart court.

The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars

How do the magnetic fields of massive stars evolve over time? Are their gyrochronological ages consistent with ages inferred from evolutionary tracks? Why do most stars predicted to host Centrifugal Magnetospheres (CMs) display no H$\alpha$ emission? Does plasma escape from CMs via centrifugal breakout events, or by a steady-state leakage mechanism? This thesis investigates these questions via a population study with a sample of 51 magnetic early B-type stars. The longitudinal magnetic field \bz~was measured from Least Squares Deconvolution profiles extracted from high-resolution spectropolarimetric data. New rotational periods $P_{\rm rot}$ were determined for 15 stars from \bz, leaving only 3 stars for which $P_{\rm rot}$ is unknown. Projected rotational velocities \vsini~were measured from multiple spectral lines. Effective temperatures and surface gravities were measured via ionization balances and line profile fitting of H Balmer lines. Fundamental physical parameters, \bz, \vsini, and $P_{\rm rot}$ were then used to determine radii, masses, ages, dipole oblique rotator model, stellar wind, magnetospheric, and spindown parameters using a Monte Carlo approach that self-consistently calculates all parameters while accounting for all available constraints on stellar properties. Dipole magnetic field strengths $B_{\rm d}$ follow a log-normal distribution similar to that of Ap stars, and decline over time in a fashion consistent with the expected conservation of fossil magnetic flux. $P_{\rm rot}$ increases with fractional main sequence age, mass, and $B_{\rm d}$, as expected from magnetospheric braking. However, comparison of evolutionary track ages to maximum spindown ages $t_{\rm S,max}$ shows that initial rotation fractions may be far below critical for stars with $M_*>10 M_\odot$. Computing $t_{\rm S,max}$ with different mass-loss prescriptions indicates that the mass-loss rates of B-type stars are likely much lower than expected from extrapolation from O-type stars. Stars with H$\alpha$ in emission and absorption occupy distinct regions in the updated rotation-magnetic confinement diagram: H$\alpha$-bright stars are found to be younger, more rapidly rotating, and more strongly magnetized than the general population. Emission strength is sensitive both to the volume of the CM and to the mass-loss rate, favouring leakage over centrifugal breakout.