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Le buste de Giuseppe Verdi , œuvre d’Antonio Ugo, admire l'architecture des bâtiments situés sur la place qui porte son nom. C’est là que se trouve le magnifique théâtre de Palerme dont je vous parlerai ultérieurement.
The bust of Giuseppe Verdi, work of Antonio Ugo, admires the architecture of the buildings located in the square that bears his name. This is where the magnificent Palermo Theater is located which I will tell you about later.
Un grand merci pour vos favoris, commentaires et encouragements toujours très appréciés.
Many thanks for your much appreciated favorites and comments.
Giuseppe Palizzi (Lanciano (Chieti) 1812 - 1888 Passy (France)) - Farmhouse in the countryside (1870-1880) oil on canvas size 38 x 59 cm - Gallery of Modern Art Paolo and Adele Giannoni - Novara
Nel 1836 s'iscrive all'Istituto d'Arte di Napoli, è allievo di Pitloo, poi di Smargiassi. Dipinge "Scena Romantica", 1838, e "Pia de' Tolomei", 1839. All'inizio del 1845 va in Francia. Nel 1848 al Salon espone "Accampamento di zingari". Vive nell'ambiente dei Barbizonniers dei quali subisce l'influenza. Nel 1854 è a Napoli e da un nuovo indirizzo alla pittura del fratello Filippo. Nel 1855 torna a Parigi e all'Esposizione Universale espone "Une Vendange e Charbonniere dans la foret de Fontainebleau".
In 1836 he enrolled at the Art Institute of Naples, is a student of Pitloo, then Smargiassi. It paints "Romantic scene", 1838, and "Pia de' Tolomei", 1839. At the beginning of 1845 it goes in France. In 1848 at the Salon exhibits "Camp of Gypsies". He lives in the environment of the Barbizonniers of which suffers the influence. In 1854 he was in Naples and gives a new address to the painting of his brother Philip. In 1855 he returned to Paris and exhibited at the Exposition Universelle "Une Vendange and Charbonniere dans la foret de Fontainebleau".
GIUSEPPE GRECO 2008
CANON EOS 400D SIGMA 10/20
Please don't use this image on websites, blogs or other media without my explicit permission. © All rights reserved
Photographed outdoor in full daylight.
Ref. Garden II 084 (macro)
©WhiteAngel Photography. All rights reserved.
Dettaglio dal "compianto del cristo morto" di Nicolo' dell'Arca, chiesa di Santa Maria della Vita. Bologna. Clay.
in the heart of paris, at the wonderful sicilian restaurant respiro, giuseppe served us with a smile that brightened our day, which was grey and rainy. this moment was pure serendipity, almost magical, his comedic talent, shown between serving dishes, seemed to echo through the streets. when i noticed how the table perfectly mirrored the scene, i had to capture this fleeting moment. giuseppe, completely unaware, became a living artwork in motion, caught in a step where up and down blend seamlessly. his authenticity and energy are the true soul of this photograph.
Model: Giuseppe Fondacaro
Production : II Mostra Fotografica - Foto Amatori Gioiesi
Location: "Le Cisterne" - Gioia Tauro (RC), Italia
Photo: Giuseppe Tripodi
GIUSEPPE GRECO 2007
CANON EOS 400D CANON EF-S 18-55
Please don't use this image on websites, blogs or other media without my explicit permission. © All rights reserved
Ogni qualvolta vado a trovarlo non posso fare a meno di rubargli qualche scatto.
Il bello è che lui, come un giovane modello,sembra assai divertito.
Se ne sta così, quasi tutto il giorno, magari aspettando qualcuno per scambiare quattro chiacchere.....
Pleiades and galactic cirrus clouds
Credit: Giuseppe Donatiello
After decades of investigations, there are still those who claim that the cirrus clouds in the Pleiades are remnants of their formation. How true will it be?
About 135 pc distant and with an estimated age of 130 ±20 Myr (Barrado y Navascués et al. 2004), M45 is certainly a young-than-average open cluster, but not as young as believed.
The higher mass members are: Alcyone, Electra, Atlas, Maia, Merope, Taygeta, Pleione and Celeno. Some of them are stars of class Be, however under 8 solar masses. It must be said, however, that some are binary and multiple systems, therefore the real masses of the individual components could be lower [A&A 425, L45-L48 (2004)]. The group mainly contains stars of class A and F, therefore between about 1 and 2.5 solar masses. Clearly there are red dwarfs and substellar objects such as numerous brown dwarfs.
Taking into account the estimated age, all stars with masses greater than 8 times the sun have already exploded as supernovae millions of years ago.
Some of the brightest stars are now in the process of evolving into red giants and some have already done so, as some massive white dwarfs have been discovered.
If we had observed the Pleiades a few million years ago, we would have seen a nice mix of white stars and red giants, as in some younger OCs.
Regardless, M45 could not have remnants of the original cloud since they usually last only a few million years before being swept away by the radiation pressure exerted by the most massive stars.
Those clouds, which many believe to be remnants of the original hydrogen cloud, are instead cirrus clouds belonging to the larger Taurus Molecular Cloud (TMC-1) that the cluster is now passing through. That cluster and cloud are not correlated can be seen from their reciprocal, almost opposing motions (Steven J. Gibson and Kenneth H. Nordsieck 2003 ApJ 589 362)
The Pleiades are moving towards the constellation of Orion and will still resist another 250 million years before completely disintegrating under the effects of the tidal forces exerted by the Milky Way.
Cirrus clouds only scatter the light of nearby stars.
Imaging lenses:
Pair of Tair-3S 300mm f/4.5
Imaging cameras:
Canon EOS 4000D
Mounts:
Avalon Instruments M-Zero Fast Reverse
Synta EQ5
Superstack