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Titlebook: Variability of Active Galaxies; Proceedings of a Wor Wolfgang J. Duschl,Stefan J. Wagner,Max Camenzind Conference proceedings 1991 Springer

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31#
發(fā)表于 2025-3-26 21:25:54 | 只看該作者
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
32#
發(fā)表于 2025-3-27 01:35:07 | 只看該作者
Esko Valtaoja ‘a(chǎn)lmost 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, h
33#
發(fā)表于 2025-3-27 08:06:30 | 只看該作者
34#
發(fā)表于 2025-3-27 10:34:52 | 只看該作者
35#
發(fā)表于 2025-3-27 16:32:42 | 只看該作者
36#
發(fā)表于 2025-3-27 19:28:38 | 只看該作者
37#
發(fā)表于 2025-3-27 23:30:02 | 只看該作者
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
38#
發(fā)表于 2025-3-28 02:13:40 | 只看該作者
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
39#
發(fā)表于 2025-3-28 07:16:26 | 只看該作者
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
40#
發(fā)表于 2025-3-28 13:17:50 | 只看該作者
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 ? to 5000 ? to within ±1 day. This pattern is difficult to reconcile with models where the “big-bump” represents th
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