我正派 发表于 2025-3-26 21:25:54
Hagai Netzers to the middle part of his account of Hardy’s career). My own focus will be on the changed attitude these novels display towards his readers. For the two novels which followed his ‘failure’ at tragedy Hardy attempted to provide his readers with the gentle amusement they appeared to crave. In the th异教徒 发表于 2025-3-27 01:35:07
Esko Valtaoja ‘almost unique in the English nineteenth-century novel’, observes a recent critic, ‘in that he creates women who are sexually exciting’ (Stubbs, 1979: 65). In many ways, of course, his writing remains rooted in the Victorian period. But in some respects at least, as I argue later in this chapter, hacrimony 发表于 2025-3-27 08:06:30
http://reply.papertrans.cn/99/9805/980498/980498_33.pngIrritate 发表于 2025-3-27 10:34:52
http://reply.papertrans.cn/99/9805/980498/980498_34.pngagitate 发表于 2025-3-27 16:32:42
http://reply.papertrans.cn/99/9805/980498/980498_35.pngHALL 发表于 2025-3-27 19:28:38
http://reply.papertrans.cn/99/9805/980498/980498_36.png不确定 发表于 2025-3-27 23:30:02
Bradley M. Petersongrew into a full designmethodology with a software system supporting it. ..Hardware-Software Co-Design of Embedded Systems: The POLISApproach. is intended to gi978-1-4613-7808-2978-1-4615-6127-9Series ISSN 0893-3405宣传 发表于 2025-3-28 02:13:40
A. Ger de Bruynal-variable methods, in particular, the atomic decomposition of elements in Hardy spaces and his constructive proof of the Fefferman-Stein decomposition of BMO 978-4-431-67999-8978-4-431-67905-9Series ISSN 1439-7382 Series E-ISSN 2196-9922较早 发表于 2025-3-28 07:16:26
Have all questions been asked?,strate, that a rather moderate flux of neutrinos, at a level of only a few percent to a few tens of percent of the electromagnetic flux changes the internal structure of low mass stars drastically. The stars expand, due to internal heating and begin to look like subgiants or giants. Such stars, expo行为 发表于 2025-3-28 13:17:50
Mapping the BLR in NGC 5548 & NGC 4151,aneously in both galaxies ruling-out the possibility that radial motions play a significant role in the velocity field of the BLR. The continuum variations are simultaneous from ≃ 1300 Å to 5000 Å to within ±1 day. This pattern is difficult to reconcile with models where the “big-bump” represents th