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Titlebook: Accretion Disks — New Aspects; Proceedings of the E Emmi Meyer-Hofmeister,Henk Spruit Conference proceedings 1997 Springer-Verlag Berlin He

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21#
發(fā)表于 2025-3-25 05:16:49 | 只看該作者
Radiation transfer in disks of CVs,ce1975. His research team at Boeing demonstrated the first GaAs/GaSb tandem concentrator solar cell in 1989 with a world record energy conversion efficiency of 35?, garnering awards from Boeing and NASA. He has978-3-031-30814-7978-3-031-30812-3
22#
發(fā)表于 2025-3-25 10:10:06 | 只看該作者
Comparison of different models for the UV-X emission of AGN,r practical value explained..What You‘ll Learn.Low-Level Programming.?teaches programmers to:.Freely write in assembly language.Understand the programming model of Intel 64.Write maintainable and robust code in978-1-4842-2402-1978-1-4842-2403-8
23#
發(fā)表于 2025-3-25 12:27:07 | 只看該作者
24#
發(fā)表于 2025-3-25 16:34:52 | 只看該作者
978-3-662-14142-7Springer-Verlag Berlin Heidelberg 1997
25#
發(fā)表于 2025-3-25 23:05:15 | 只看該作者
Accretion Disks — New Aspects978-3-540-68715-3Series ISSN 0075-8450 Series E-ISSN 1616-6361
26#
發(fā)表于 2025-3-26 00:54:55 | 只看該作者
27#
發(fā)表于 2025-3-26 06:41:24 | 只看該作者
Morgan Schellenberg,Kenji Inabae involved and describe different models proposed to account for them. We schematize these models in a simple way, and compute the emitted spectra, insisting on their main characteristics and on their differences.
28#
發(fā)表于 2025-3-26 09:21:40 | 只看該作者
29#
發(fā)表于 2025-3-26 12:59:22 | 只看該作者
Family Oziidae Dana, 1851 (Forceps Crabs) and those of X-ray binaries containing a black hole (black-hole XBs). The X-ray spectra of these systems change their characteristics with the mass accretion rate. At high X-ray luminosities, typically . .>10. erg sec., soft thermal emission from the accretion disk dominates. There is a distinct di
30#
發(fā)表于 2025-3-26 19:50:15 | 只看該作者
Anatomy of Craniocervical Junctionuring its four successive hard X-ray outbursts in 1990–1994 were studied in details. We suggest that the mechanism of GX 339-4 outbursts is triggering of the irradiation — driven instability in the low mass binary system.
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