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Comment inscrire l'absolu dans l'immuable ? La Loi Royale de Frédéric III établissant une monarchie absolue au Danemark (1665)
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Cumes : la nécropole de la porte Médiane des fortifications septentrionales
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Issues at Stake in Poetic Commentary in Medieval Japan
No full textInternational audienceIn order to understand the issues at stake in poetic commentary in medieval Japan, this article examines one of the oldest commentaries in the Japanese tradition, the Kenchū mikkan or “Secret investigations of Kenshō’s commentary [on Kokin waka shū ]”, a commentary on the first anthology of Japanese poetry compiled by imperial order, around 905. The Kenchū mikkan dates from 1221. It is a double commentary by two poets, among the most important in the Japanese tradition, who belonged to two rival poetic schools. The first, Kenshō (1130?–1209), belonged to the Rokujō school, while the second, Fujiwara no Teika (1162–1241), was head of the Mikohidari school. Around 1183, Kenshō wrote a commentary entitled Kokin hichū shō “Notes on the secret commentaries of the Kokin [waka shū ]”, in which he comments on 410 of the 1111 poems of the imperial anthology. In 1221, Teika added his own commentaries to Kenshō’s text: Kenchū mikkan is the title given to this double commentary. In the article we examine the entire section dedicated to the Laments, that is to say, 12 poems and their commentaries. Reading this section will enable us to understand the specific points of the two poets’ commentaries, and therefore what they considered to be the essential information to be conveyed
Anne P. Alwis, Narrating Martyrdom. Rewriting Late-Antique Virgin Martyrs in Byzantium. Translated with introduction and notes by Anne P. Alwis (Translated Texts for Byzantinists 9). – Liverpool University Press, Liverpool 2020. 21,5 x 15,5. 210 p. Price: 95 GBP. ISBN 978-1-78962-155-6.
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A New Concepts of Settlement in Ninevite 5 Upper Mesopotamia. The Case of Bash Tapa
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Interactions et évolutions textuelles : des aventures d'une légende à une réflexion générale
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Zur Kritik des autoritären Liberalismus. Heller gegen Schmitt im Jahre 1932
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Fouille des tombes néolithiques du site de Houtaomuga à Da'an, Jilin
No full textJilin daxue Bianjiang kaogu yanjiu zhongxin 吉林大学边疆考古研究中心 et Jilin sheng wenwu kaogu yanjiu suo 吉林省文物考古研究所, « Jilin Da’an Houtaomuga yizhi Xinshiqi shidai muzang fajue jianbao 吉林大安后套木嘎遗址新石器时代墓葬发掘简报 », Wenwu, 2023, nᵒ 11, p. 28‑40
Zheng Zhenxiang : disparition d’un monstre sacré de l’archéologie chinoise
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A Case Study of Gas Impacted by Black-hole Jets with the JWST: Outflows, Bow Shocks, and High Excitation of the Gas in the Galaxy IC 5063
No full textInternational audienceWe present James Webb Space Telescope MIRI data of the inner ∼3 × 2 kpc2 of the galaxy IC 5063, in which the jets of a supermassive black hole interact with the gaseous disk they are crossing. Jet-driven outflows were known to be initiated along or near the jet path and to modify the stability of molecular clouds, possibly altering their star formation properties. The MIRI data, of unprecedented resolution and sensitivity in the infrared, now reveal that there are more than 10 discrete regions with outflows, nearly doubling the number of such known regions. Outflows exist near the radio lobes, at the nucleus, in a biconical structure perpendicular to the jet, and in a bubble moving against the disk. In some of them, velocities above escape velocity are observed. Stratification is also observed, with higher ionization or excitation gas attaining higher velocities. More outflows and bow shocks, found further away from the nucleus than the radio lobes, in regions without significant radio emission, reveal the existence of past or weak radio jets that interacted with the interstellar medium. The coincidence of the bow shocks with the optical extended emission line region (EELR) suggests that the jets also contributed to the gas ionization. Maps of the H2 gas excitation temperature, T ex, indicate that the molecular gas is most excited in regions with radio emission. There, T ex is >100 K higher than in the EELR interior. We argue that a combination of jet-related shocks and cosmic rays is likely responsible for this excess molecular gas excitation