La relación de las exequías de Carlos III en Roma y el nuevo gusto neoclásico

El fallecimiento de Carlos III en diciembre de 1788 fue conmemorado en la Roma de Pío VI con unas exequias oficiales españolas organizadas por el embajador José Nicolás de Azara y por un funeral ordenado por el Papa. Azara aprovechó la ocasión para materializar en dicha función fúnebre sus radicales principios neoclásicos. Paralelamente, ambas ceremonias efímeras se fijaron mediante una serie de lujosas publicaciones en las que intervino decisivamente el impresor más característico del Neoclasicismo: Gimbattista Bodoni. Las exequias de Carlos III en Roma fueron la obra de un intelectual. Son producto de la Roma cosmopolita de los años ochenta del siglo XVIII, foco de atracción para artistas, aficionados, coleccionistas e inteligentes en las artes.

Electron collisions with Fe-peak elements: Forbidden transitions between the low lying valence states 3d6, 3d54s, and 3d54p of Fe III:

Effective collision strengths are presented for the Fe-peak element Fe III at electron temperatures (Te in degrees Kelvin) in the range 2 × 103 to 1 × 106. Forbidden transitions results are given between the 3d6, 3d54s, and the 3d54p manifolds applicable to the modeling of laboratory and astrophysical plasmas.

High-resolution spectroscopic observations of B-type stars from the Edinburgh-Cape Survey - III. Completion of a magnitude range limited survey

High spectral resolution (R similar to 40 000) and signal-to- noise ratio observations of five high Galactic latitude early- type stars taken from the Edinburgh-Cape (EC) Faint Blue Object Survey are presented. These were required to complete a magnitude range-limited survey of young B-type objects with 11 <V <15. Of the five stars, four were rejected on the grounds that they are either subluminous (subdwarf or horizontal branch), were part of a binary system or possessed colours later than the (U - B) = -0.5 cut-off employed. The remaining star in the data set, EC 19596-5356, is found to exhibit normal young B-type stellar properties. A kinematic analysis reveals that an origin in the Galactic disc appears likely for all the stars in the sample. Some statistics are drawn about the number density of young stars in the Galactic halo.