认为
发表于 2025-3-25 07:52:57
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有机体
发表于 2025-3-25 11:45:05
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消音器
发表于 2025-3-25 19:00:13
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织物
发表于 2025-3-25 21:05:30
Ali E. Karakaya,Semra Sardas,Sema Burgazces discovered by the COS-B satellite..32 low latitude (|.| < 5°) IPC fields, mosaic-arranged to cover the few-square-degrees COS-B error circles, yielded 30 soft X-ray sources, the fluxes of which range from ~ 1/100 to few UFU, and no diffuse features..While the density of ~ 1 source/IPC field is c
Seminar
发表于 2025-3-26 02:28:13
Using , for Two-Phase Flow in Porous Media COS-B. The consistency of the two datasets is discussed; while a satisfying general agreement is observed, a few distinct discrepancies point to possible time variations within the compact source component of the total galactic emission. The bulk of emission appears very well correlated to the colu
袖章
发表于 2025-3-26 05:38:23
Background for Advances in Data Base Theoryal measurements are now available at those energies, where the contribution from π°-decay gamma rays can be neglected. The high MeV-fluxes observed in both parts of the Galaxy are an indication of either a strong electron induced component or a high contribution from unresolved sources. Several inte
somnambulism
发表于 2025-3-26 08:42:29
Eliminating Cycles in Database Schemas from galaxy counts. It is found that to a good approximation the gamma-ray intensity is proportional to the total gas column density, and on this basis a map of the angular distribution of local molecular hydrogen at intermediate latitudes is presented. Comparing this with a simular map produced fr
ACTIN
发表于 2025-3-26 15:31:34
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并置
发表于 2025-3-26 19:28:59
https://doi.org/10.1007/978-1-4613-4024-9ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hum
开花期女
发表于 2025-3-27 00:49:30
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