966 resultados para 1ST STARS
Resumo:
The eighth volume of College Papers contains original documents dating from 1815 to 1819, spanning the tenures of president John Thornton Kirkland and treasurer John Davis. Much of the volume consists of general administrative correspondence exchanged between Kirkland and Davis. It also contains a document from 1820.
Resumo:
The ninth volume of College Papers contains original documents dating from 1819 to 1821, spanning the tenures of president John Thornton Kirkland and treasurer John Davis, as well as correspondence between Davis and Steward Stephen Higginson. Much of the volume consists of general administrative correspondence exchanged between Kirkland and Davis. It also contains an early 20th century typewritten document.
Resumo:
The tenth volume of College Papers contains original documents dating from 1821 to 1824, spanning the tenures of president John Thornton Kirkland and treasurer John Davis. Much of the volume consists of general administrative correspondence exchanged between Kirkland and Davis, as well as correspondence between Davis and Steward Stephen Higginson. It also contains a printed document from 1831, during the tenure of president Josiah Quincy.
Resumo:
The eleventh volume of College Papers contains original documents from 1824 to 1825, spanning the tenures of president John Thornton Kirkland and treasurer John Davis. Much of the volume consists of general administrative correspondence exchanged between Kirkland and Davis, as well as correspondence between Davis and Steward Stephen Higginson.
Resumo:
In this thesis, the origin of large-scale structures in hot star winds, believed to be responsible for the presence of discrete absorption components (DACs) in the absorption troughs of ultraviolet resonance lines, is constrained using both observations and numerical simulations. These structures are understood as arising from bright regions on the stellar surface, although their physical cause remains unknown. First, we use high quality circular spectropolarimetric observations of 13 well-studied OB stars to evaluate the potential role of dipolar magnetic fields in producing DACs. We perform longitudinal field measurements and place limits on the field strength using Bayesian inference, assuming that it is dipolar. No magnetic field was detected within this sample. The derived constraints statistically refute any significant dynamical influence from a magnetic dipole on the wind for all of these stars, ruling out such fields as a cause for DACs. Second, we perform numerical simulations using bright spots constrained by broadband optical photometric observations. We calculate hydrodynamical wind models using three sets of spot sizes and strengths. Co-rotating interaction regions are yielded in each model, and radiative transfer shows that the properties of the variations in the UV resonance lines synthesized from these models are consistent with those found in observed UV spectra, establishing the first consistent link between UV spectroscopic line profile variability and photometric variations and thus supporting the bright spot paradigm (BSP). Finally, we develop and apply a phenomenological model to quantify the measurable effects co-rotating bright spots would have on broadband optical photometry and on the profiles of photopheric lines in optical spectra. This model can be used to evaluate the existence of these spots, and, in the event of their detection, characterize them. Furthermore, a tentative spot evolution model is presented. A preliminary analysis of its output, compared to the observed photometric variations of xi Persei, suggests the possible existence of “active longitudes” on the surface of this star. Future work will expand the range of observational diagnostics that can be interpreted within the BSP, and link phenomenology (bright spots) to physical processes (magnetic spots or non-radial pulsations).
