Baalbec. 1844. Petit et Grand Temple : [photographie] / Joseph Philibert Girault de Prangey

Ancien possesseur : Simony, Charles de (Cte Anne Marie Charles de)

[Voyage en Italie : 1824-1830]. , Forum. Temple de Jupiter : [plan d'ensemble du temple et d'une partie du forum] : [dessin] / h. L. [Henri Labrouste]

Référence bibliographique : Weigert, 370

[Voyage en Italie : 1824-1830]. , Coupe du Temple de Jupiter. Coupe du Forum. Sur une Echelle de 001 PM : [coupe longitudinale sur le temple, coupe transversale sur le forum] : [dessin] / h. L. [Henri Labrouste]

Référence bibliographique : Weigert, 371

[Pouzzoles. Temple de Jupiter Serapis]

Référence bibliographique : Weigert, 469

[Pouzzoles. Temple de Jupiter Serapis]

Référence bibliographique : Weigert, 470

Tempio di Giove e foro a Pompei : [vue générale du temple de Jupiter et du forum à Pompéi] : [peinture]

Collectionneur : Lesouëf, Auguste (1829-1906)

[Ostie. Tempio di Giove Ottimo Massimo]

Référence bibliographique : Weigert, 302

[Ostie. Tempio di Giove Ottimo Massimo]

Référence bibliographique : Weigert, 303

[Ostie. Tempio di Giove Ottimo Massimo]

Référence bibliographique : Weigert, 304

[Ostie. Tempio di Giove Ottimo Massimo]

Référence bibliographique : Weigert, 305

Baalbec. 1843. Carrières à l'O. : [photographie] / Joseph Philibert Girault de Prangey

Ancien possesseur : Simony, Charles de (Cte Anne Marie Charles de)

[Illustrations de Le Temple de Gnide] / Le Mire Noël, grav. ; Montesquieu, aut. du texte

Comprend : [Pl. en reg. p.1. Premier chant : Vénus et Vulcain, sur le lit nuptial, devant l'assemblée des Dieux et des nymphes (dont Mercure et Zeus).] Sa robe fuit ses genoux, la toile vole... [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407] ; [Pl. en reg. p.25. Second chant : une coquette, venue à Gnide, reçoit l'oracle de Vénus. ] Tu mourras accablée de refus et de mépris. [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407] ; [Pl. en reg. p.31. Troisième chant : Vénus et les trois Grâces couronnent la beauté de Thémire.] Elle appella les Grâces : Allez la couronner... [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407] ; [Pl. en reg. p.45. Quatrième chant : Thémire et son amant.] Une nuit que j'étois dans cet état tranquille... [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407] ; [Pl. en reg. p.61. Cinquième chant : Aristée et Camille.] Je sens couler mes larmes... [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407] ; [Pl. en reg. p.73. Sixième chant : la Fureur jette un serpent dans le coeur de l'amant de Thémire.] Elle détacha un de ses serpents. .. [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407] ; [Pl. en reg. p.87. Septième chant : l'Amour se cache sous les jupes de Thémire.] Il se cacaha sous ses genoux, je le suivis... [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407] ; [Pl. en reg. p.99 : Céphise coupe les aîles de l'Amour.] Elle coupa le sommet des aîles de l'Amour... [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407] ; [Pl. en reg. p.102 : Jupiter envoie Cupidon auprès de Vénus pour que l'amour de la déesse fasse repousser les aîles de l'Amour.] La chaleur va les faire renaître... [Cote : 4 ° Z Don 205 (39)/Microfilm R 122407]

The Last Missionary to Leave the Temple Should Turn Off the Light Sociological Remarks on the Decline of Japanese ""Immigrant"" Buddhism in Brazil

Empirical data indicate that the so-called ""Buddhism of yellow color"" that is predominantly associated with Japanese ""immigrant"" Buddhism, is constantly in decline in terms of ""explicit"" adherents. After some methodological observations, this article gives an overview of the relevant statistical data. The last part discusses possible reasons for these negative dynamics, referring to causes within Buddhist institutions, the ethnic community, and at the level of the individual.

Physical and dynamical characterization of (5201) Ferraz-Mello, a possible extinct Jupiter family comet

Context. The subject of asteroids in cometary orbits (ACOs) has been of growing interest lately. These objects have the orbital characteristics typical of comets, but are asteroidal in appearance, i.e., show no signs of a coma at any part of their orbits. At least a fraction of these objects are thought to be comets that have either exhausted all their volatile content or developed a refractory crust that prevents sublimation. In particular, the asteroid ( 5201) Ferraz-Mello has, since its discovery, been suspected to be an extinct Jupiter family comet due to the peculiar nature of its orbit. Aims. The aim of this work is to put constraints on the possible origin of ( 5201) Ferraz-Mello by means of spectroscopic characterization and a study of the dynamics of this asteroid. Methods. We used the SOAR Optical Imager (SOI) to obtain observations of ( 5201) Ferraz-Mello using four SDSS filters. These observations were compared to asteroids listed in the Sloan Moving objects catalog and also to photometry of cometary nuclei, Centaurs, and TNOs. The orbital evolution of ( 5201) Ferraz-Mello and of a sample of asteroids and comets that are close to that object in the a - e plane were simulated using a pure N-body code for 4 000 years forward and 4 000 years backward in time. Results. The reflectance spectrum obtained from its colors in the SDSS system is unusual, with a steep spectral gradient that is comparable to TNOs and Centaurs, but with an increase in the reflectance in the g band that is not common in those populations. A similar behavior is seen in cometary nuclei that were observed in the presence of a faint dust coma. The dynamical results confirm the very chaotic evolution found previously and its dynamical similarity to the chaotic evolution of some comets. The asteroid is situated in the very stochastic layer at the border of the 2/1 resonance, and it has a very short Lyapunov time ( 30 - 40) years. Together, the spectral characteristcs and the dynamical evolution suggest that ( 5201) Ferraz-Mello is a dormant or extinct comet.

Transiting exoplanets from the CoRoT space mission XVI. CoRoT-14b: an unusually dense very hot Jupiter

In this paper, the CoRoT Exoplanet Science Team announces its 14th discovery. Herein, we discuss the observations and analyses that allowed us to derive the parameters of this system: a hot Jupiter with a mass of 7.6 +/- 0.6 Jupiter masses orbiting a solar-type star (F9V) with a period of only 1.5 d, less than 5 stellar radii from its parent star. It is unusual for such a massive planet to have such a small orbit: only one other known higher mass exoplanet orbits with a shorter period.