Jeanne de Montfort; époque guerrière: 1342;

Mode of access: Internet.

Guida per la città di Padova : all' amico delle belle arti.

Includes indexes.

Relazioni delle memorie lette nell' I.R. Accademia di scienze, lettere ed arti in Padova negli anni MDCCCXL-MDCCCXLI.

Port. of Gralilei.

Memoria sulla libertà del commercio, diretta a risolvere il problema proposto dall'Accademia di Padova sullo stesso argomento.

In Scrittori classici italiani di economia politica. Milano, 1805. 22 cm. [v. 46] Parte moderna, v. 39, p. [7]-76.

Nuova guida pei forestieri amatori delle belle arti per conoscere facilmente le cose piu ̀notabili che si trovano in Padova.

Includes index.

Annali della città di Padova /

945.312 G287a v.1 cop.2: University of Illinois Library bookplate "From the library of Conte Antonio Cavagna Sangiuliani di Gualdana Lazelada di Bereguardo, purchased 1921" on the inside front cover.

Notizie storiche circa li pubblici professori nello Studio di Padova scelti dall'Ordine di San Domenico /

Signatures: A-M���, N-N², F³-F⁸. Signatures F³-F⁸ were mis-lettered and should read N³-N⁸.

Cronaca d'Orvieto dal 1342 al 1363 /

Reprint of the 1865 ed. published by G. Daelli, Milan, which was issued as v. 58 of Biblioteca rara.

Monumenti della Università di Padova, 1318-1405 /

Reprint of the 1888 ed. published by Tip. del Seminario, Padua, which was issued as no. 1 of Studi editi dalla Università di Padova a commemorare l'ottavo centenario dalla origine della Università di Bologna.

Bollettino del Museo civico di Padova.

"Revista Padovana di arte antica e moderna numismatica araldica storia e letteratura."

Icklingham papers. Manors, churches, townlands and antiquities of Icklingham, together with the text and translation of the Berners' manorial accounts, 1342-3,

Mode of access: Internet.

New Galactic star clusters discovered in the VVV survey

Context. VISTA Variables in the Via Lactea (VVV) is one of the six ESO Public Surveys operating on the new 4-m Visible and Infrared Survey Telescope for Astronomy (VISTA). VVV is scanning the Milky Way bulge and an adjacent section of the disk, where star formation activity is high. One of the principal goals of the VVV Survey is to find new star clusters of different ages. Aims. In order to trace the early epochs of star cluster formation we concentrated our search in the directions to those of known star formation regions, masers, radio, and infrared sources. Methods. The disk area covered by VVV was visually inspected using the pipeline processed and calibrated K(S)-band tile images for stellar over-densities. Subsequently, we examined the composite JHK(S) and ZJK(S) color images of each candidate. PSF photometry of 15 x 15 arcmin fields centered on the candidates was then performed on the Cambridge Astronomy Survey Unit reduced images. After statistical field-star decontamination, color-magnitude and color-color diagrams were constructed and analyzed. Results. We report the discovery of 96 new infrared open clusters and stellar groups. Most of the new cluster candidates are faint and compact (with small angular sizes), highly reddened, and younger than 5 Myr. For relatively well populated cluster candidates we derived their fundamental parameters such as reddening, distance, and age by fitting the solar-metallicity Padova isochrones to the color-magnitude diagrams.

Microstructural Effects of Sn Addition to Fe(2)O(3) Thin Films

The influence of Sri in Fe(2)O(3) thin films is addressed. The presence of the tin ions decreases the Fe(2)O(3) particle sizes and surface roughness decreasing of the films` surface is observed as a consequence. X-ray diffraction and atomic force microscopy measurements together with literature results support this phenomenon to be related to the segregation of the additive onto the surface and consequently surface energy decrease, which constitutes the driving force for the microstructure modification, similarly to results previously obtained for powders with same compositions. The effect of the anions introduced in the system as counter-ions of the precursors is also discussed.

High Carbon Ferro-Chromium by Self-Reducing Process

This paper discusses the effects of temperature, addition of ferro-silicon and fluxing agents for the production of high carbon ferro-chromium by self-reducing process. The use of self-reducing agglomerates for ferro-alloys production is becoming an emerging processing technology due to lowering the electric energy consumption and improving the metal recovery in comparison with traditional ones. The self-reducing pellets were composed by chromite, petroleum coke, cement and small (0.1% - 2%) addition of ferro-silicon. The slag composition was adjusted by addition of fluxing agents. The reduction of pellets was carried out at 1773K (1500 degrees C), 1823K (1550 degrees C) and 1873K (1600 degrees C) by using induction furnace. The products obtained, containing slag and metallic phases, were analyzed by scanning electron microscopy and chemical analyses (XEDS). By increasing temperature from 1773K to 1823K large effect on the reduction time was observed. It decreased from 30 minutes to 10 minutes, for reaching around 0.98 reduction fraction. No significant effect on reduction time was observed when the reduction temperature was increased from 1823K to 1873K. At 1773K, the addition of 2% of ferro-silicon in the pellet resulted in an increasing reaction rate of around 6 times, in comparison with agglomerate without this addition. The addition of fluxing agents (silica and hydrated lime) has effect on reduction time (inverse relationship) and the pellets become less porous after reduction.