Incumbent
发表于 2025-3-23 10:36:05
Dimitrios Millas,Oliver Porth,Rony Keppensraneous social organizations than anything biological, no longer serve, but rather obstruct. Every science is guided by its current models, even ones that are implicit, and even if the investigator disowns them, and purports to base his conclusions solely on empirical grounds. The dominant models al
glomeruli
发表于 2025-3-23 17:14:53
Z. Meliani,O. Hervets attractions to and repulsions from chance. In this approach stages of knowledge about the outcome, from ignorance in the pre-outcome period, to certainty in the post-outcome period, are used to identify the necessarily different episodes in the decision makers’ future from the point of embarking o
ostracize
发表于 2025-3-23 20:22:01
raneous social organizations than anything biological, no longer serve, but rather obstruct. Every science is guided by its current models, even ones that are implicit, and even if the investigator disowns them, and purports to base his conclusions solely on empirical grounds. The dominant models al
强制性
发表于 2025-3-24 01:31:08
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交响乐
发表于 2025-3-24 03:25:29
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watertight,
发表于 2025-3-24 10:24:23
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fleeting
发表于 2025-3-24 12:48:07
Brunella Nisini,Simone Antoniucci,Juan Manuel Alcalá,Teresa Giannini,Carlo Felice Manara,Antonella N such dangerous ideas is actively prevented. This book provides a detailed map of this astonishing struggle in today’s America—a struggle many had thought was done and dusted with the onset of the Enlightenment978-94-007-3809-6978-94-007-1808-1Series ISSN 1879-7229 Series E-ISSN 1879-7237
Criteria
发表于 2025-3-24 16:02:52
1570-6591 ults on the impact of the study of protostellar jets on other jet studies in particular on relativistic jets. As a matter of fact, it is time for a new network..978-3-030-14130-1978-3-030-14128-8Series ISSN 1570-6591 Series E-ISSN 1570-6605
专横
发表于 2025-3-24 20:31:25
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FLIP
发表于 2025-3-25 02:56:41
Radiation Magnetohydrodynamic Models and Spectral Signatures of Plasma Flows Accreting onto Classicashocked plasma is partially absorbed by the unshocked accretion column, and this might explain the excess of X-ray flux predicted by MHD models which do not include absorption effects. Moreover, due to the absorption of radiation, the pre-shock downfalling accreted material is gradually heated up to