Picaronas y alcahuetes ó La mancebía de Valencia : apuntes para la historia de la prostitucion desde principios del siglo XIV hasta poco antes de la abolición de los fueros...

Indice

La France sous Louis XV (1715-1774)

v. 1. Introduction: Règne de Louis XIV. La régence.--v. 2. La régence. Ministère du duc de Bourbon. Ministère de Fleury de 1727 à 1732.--v. 3. Ministère de Fleury de 1732 à 1743. Madame de Chateauroux de 1743 à 1745. Madame de Pompadour de 1745 à 1746.--v. 4. Madame de Pompadour de 1746 à 1757.--v. 5. Madame de Pompadour de 1757 à 1763.--v. 6. Madame de Pompadour de 1763 au 15 avril 1764. Ministère du duc de Choiseul, de 1764 au 24 décembre 1770. Madame du Barry, du 24 décembre 1770 à la mort de Louis XV.

La pittura lombarda dal XIV al XVI secolo, preceduta da uno studio teorico su la moralità estetica /

"Indice degli artisti" : p. xv-xvi.

Bullarii romani continuatio summorum pontificum Clementis XIII, Clementis XIV, Pii VI, Pii VII, Leonis XII, Pii VIII [et Gregorii XVI] : constitutiones, literas in forma brevis epistolas ad principes viros et alios atque allocutiones complectens /

Contiene: T. I : Continens pontificatus Clementis XIII. Annum primum, et secundum (1835. XXVIII, 411 p.) -- T. II : Annum tertium ad sextum (1837. XXII, 550 p.) -- T. III : Clementis XIII. Septimum ad undecimum (1838. XXII, 591 p.) -- T. IV : Clementis XIV. Primum ad sextum (1841. XXVII, 806 p.) -- T. V : Pii VI. Annum primum ad tertium (1842. XIX, 490 p.) -- T. VI : Quartum ad octavum (1843. XXIV, 626 p.) -- T. VII : Annum nonum ad duodecimum (1843. XVII, 714 p.) -- T. VIII : Pii VI, [annum] XIII ad XVI (1844. XVII, 574 p.) -- T. IX : Annum decimum septimum ad vicesimum primum (1845. XXI, 638 p.) -- T. X: Vicesimum secundum ad vicesimum quintum (1845. XVIII, 250 p.) -- T. XI: Pii VII. Annum primum ad tertium (1846. XXI, 510 p.) -- T. XII : Pii VII. Annum quartum ad sextum (1846. XXI, 450 p.) -- T. XIII : Septimum ad sextum decimum (1847. XXIII, 488 p.) -- T. XIV: Annum decimum septimum ad octavum (1849. XII, 626 p.) -- T. XV: Annum decimum nonum ad vicesimum quartum (1853. XXIV, 650 p.) -- T. XVI: Leonis XII. Annum primum ad tertium (1854. XV, 490 p.) -- T. XVII: Annum quartum ad sextum (1855. XV, 483 p.) -- T. XVIII: Pii VIII. Annum primum et secundum (1856. XV, 168 p.) -- T. XIX: Gregorii XVI. Annum primum ad quartum (1857. XXVI, 714 p.) -- T. XX: Gregorii XVI. Annum quintum (1858)

Modern electrical theory ; supplementary chapters, chapter xv- /

A series of monographs intended to supplement, and eventually to replace the author's book, "Modern electrical theory", which consists of XIV chapters. cf. [volume 1] pages [v].

"Et occidetur virtute Domini Antichristus a Mikaele arcangelo". Paisaje y escatología en Sant Miquel de Llíria (s. XIV d. C.)

El presente articulo intenta determinar las razones por las que el santuario de Sant Miquel de Llíria, uno de los más importantes de la actual provincia de Valencia, se consagró al arcàngel guerrero. Se estudia para ello la historia de su culto en Occidente, haciendo hincapié en aspectos como su relación con los lugares elevados y la frecuente proximidad de sus santuarios con aquellos dedicados a la Virgen. Atenderemos también a aspectos fundamentales del contexto histórico, como los movimientos de renovación espiritual medievales, la influencia del médico y teólogo Arnau de Vilanova en la Valencia de principios del siglo XIV y las profecías escatológicas vinculadas a la llegada del Anticristo.

First stars XIV. Sulfur abundances in extremely metal-poor stars

Context. Precise S abundances are important in the study of the early chemical evolution of the Galaxy. In particular the site of the formation remains uncertain because, at low metallicity, the trend of this alpha-element versus [Fe/H] remains unclear. Moreover, although sulfur is not bound significantly in dust grains in the ISM, it seems to behave differently in DLAs and old metal-poor stars. Aims. We attempt a precise measurement of the S abundance in a sample of extremely metal-poor stars observed with the ESO VLT equipped with UVES, taking into account NLTE and 3D effects. Methods. The NLTE profiles of the lines of multiplet 1 of S I were computed with a version of the program MULTI, including opacity sources from ATLAS9 and based on a new model atom for S. These profiles were fitted to the observed spectra. Results. We find that sulfur in EMP stars behaves like the other alpha-elements, with [S/Fe] remaining approximately constant below [Fe/H] = -3. However, [S/Mg] seems to decrease slightly with increasing [Mg/H]. The overall abundance patterns of O, Na, Mg, Al, S, and K are most closely matched by the SN model yields by Heger & Woosley. The [S/Zn] ratio in EMP stars is solar, as also found in DLAs. We derive an upper limit to the sulfur abundance [S/Fe] < +0.5 for the ultra metal-poor star CS 22949-037. This, along with a previously reported measurement of zinc, argues against the conjecture that the light-element abundance pattern of this star (and by analogy, the hyper iron-poor stars HE 0107-5240 and HE 1327-2326) would be due to dust depletion.

Transiting exoplanets from the CoRoT space mission XV. CoRoT-15b: a brown-dwarf transiting companion

We report the discovery by the CoRoT space mission of a transiting brown dwarf orbiting a F7V star with an orbital period of 3.06 days. CoRoT-15b has a radius of 1.12(-0.15)(+0.30) R(Jup) and a mass of 63.3 +/- 4.1 M(Jup), and is thus the second transiting companion lying in the theoretical mass domain of brown dwarfs. CoRoT-15b is either very young or inflated compared to standard evolution models, a situation similar to that of M-dwarf stars orbiting close to solar-type stars. Spectroscopic constraints and an analysis of the lightcurve imply a spin period in the range 2.9-3.1 days for the central star, which is compatible with a double-synchronisation of the system.

Transiting exoplanets from the CoRoT space mission XIV. CoRoT-11b: a transiting massive ""hot-Jupiter"" in a prograde orbit around a rapidly rotating F-type star

The CoRoT exoplanet science team announces the discovery of CoRoT-11b, a fairly massive hot-Jupiter transiting a V = 12.9 mag F6 dwarf star (M(*) = 1.27 +/- 0.05 M(circle dot), R(*) = 1.37 +/- 0.03 R(circle dot), T(eff) = 6440 +/- 120 K), with an orbital period of P = 2.994329 +/- 0.000011 days and semi-major axis a = 0.0436 +/- 0.005 AU. The detection of part of the radial velocity anomaly caused by the Rossiter-McLaughlin effect shows that the transit-like events detected by CoRoT are caused by a planet-sized transiting object in a prograde orbit. The relatively high projected rotational velocity of the star (upsilon sin i(star) = 40 +/- 5 km s(-1)) places CoRoT-11 among the most rapidly rotating planet host stars discovered so far. With a planetary mass of M(p) = 2.33 +/- 0.34 M(Jup) and radius R(p) = 1.43 +/- 0.03 R(Jup), the resulting mean density of CoRoT-11b (rho(p) = 0.99 +/- 0.15 g/cm(3)) can be explained with a model for an inflated hydrogen-planet with a solar composition and a high level of energy dissipation in its interior.