Search results for " Aquila"
showing 5 items of 5 documents
La fine della carriera del praefectus Aegypti Subaziano Aquila. Per un’ipotesi sul ruolo dell’Egitto fra Caracalla e Geta
2022
Si analizzano le fonti storiografiche, papiracee ed epigrafiche relative alla lunga carriera del praefectus Aegypti Subaziano Aquila, in carica a partire dal 206 d.C., e si ipotizza che la fine della sua carriera sia da porre in relazione con il contrasto fra Caracalla e Geta scaturito al momento della successione a Settimio Severo. The historiographical, papyrus and epigraphic sources relating to the long career of the praefectus Aegypti Subaziano Aquila, in office starting from 206 AD, are analysed, and it is hypothesized that the end of his career is to be placed in relation to the conflict between Caracalla and Geta which arose in moment of succession to Septimius Severus.
La preferenza dell'habitat dell'Aquila reale, Aquila chrysaetos, in Sicilia
2009
Summer aggregation of common eagle ray, Myliobatis aquila (Chondrichthyes: Myliobatidae), in the Marine Protected Area of the Egadi Islands (southwes…
2021
Author(s): Grancagnolo, Desiree; Arculeo, Marco | Abstract: We report for the first time in Italian waters a periodic and frequent presence of a summer aggregation of common eagle ray Myliobatis aquila in the island of Marettimo (southwestern Tyrrhenian Sea), which is part of the Marine Protected Area of the Egadi Islands. These aggregation could be related to different phenomena such as reproduction, feeding or simply as a transit zone.
Multiperiodic pulsations in the Be stars NW Serpentis and V1446 Aquilae
2007
Aims.We present accurate photometric time series of two Be stars: NW Ser and V1446 Aql . Both stars were observed at the Observatorio de Sierra Nevada (Granada) in July 2003 with an automatic four-channel Strömgren photometer. We also present a preliminary theoretical study showing that the periodic variations exhibited by these stars can be due to pulsation. Methods.An exhaustive Fourier analysis together with a least-square fitting has been carried out on the time series for all four Strömgren bands. Several independent frequencies and non-periodic trends explain most of the variance. A theoretical non-adiabatic code applied to stellar models for these stars shows that g-modes are unstabl…