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Titlebook: Quantum Quenching, Annealing and Computation; Anjan Kumar Chandra,Arnab Das,Bikas K. Chakrabarti Book 2010 Springer-Verlag Berlin Heidelbe

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11#
發(fā)表于 2025-3-23 12:30:29 | 只看該作者
12#
發(fā)表于 2025-3-23 16:59:14 | 只看該作者
R.D. Somma,G. Ortizties of individual fruit bats we cannot make more refined predictions about the size and kind of fruit consumed, the extent to which animals are eaten, the nature of seasonal changes in diet, and so on. Our contention is that because the selective regimen imposed on a species through evolutionary ti
13#
發(fā)表于 2025-3-23 22:01:23 | 只看該作者
14#
發(fā)表于 2025-3-23 23:54:43 | 只看該作者
U. Divakaran,V. Mukherjee,A. Dutta,D. Senmportant species reared at this time was the carp, which by 1890 was found throughout North America, thanks to the development of railroads and fish transport cars. Other species were raised as well, however, so that by 1873 a railroad car containing 300,000 fish of 10 species was on its way to Cali
15#
發(fā)表于 2025-3-24 03:10:00 | 只看該作者
C. De Grandi,A. Polkovnikovmportant species reared at this time was the carp, which by 1890 was found throughout North America, thanks to the development of railroads and fish transport cars. Other species were raised as well, however, so that by 1873 a railroad car containing 300,000 fish of 10 species was on its way to Cali
16#
發(fā)表于 2025-3-24 06:47:42 | 只看該作者
17#
發(fā)表于 2025-3-24 10:55:12 | 只看該作者
18#
發(fā)表于 2025-3-24 16:18:01 | 只看該作者
19#
發(fā)表于 2025-3-24 22:32:18 | 只看該作者
V. Subrahmanyamth the observations and the .-body models strongly indicate that the long-period blue-straggler binaries—which dominate the NGC 188 blue-straggler population—are formed by asymptotic-giant (primarily) and red-giant mass transfer onto main-sequence stars. The models suggest that the few non-velocity-
20#
發(fā)表于 2025-3-25 02:17:36 | 只看該作者
S. Tanaka,M. Hirano,S. Miyashitath the observations and the .-body models strongly indicate that the long-period blue-straggler binaries—which dominate the NGC 188 blue-straggler population—are formed by asymptotic-giant (primarily) and red-giant mass transfer onto main-sequence stars. The models suggest that the few non-velocity-
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