Titlebook: Hochwertiger Grauguß und die physikalisch-metallurgischen Grundlagen seiner Herstellung; Eugen Piwowarsky Book 1929 Julius Springer in Ber

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书目名称Hochwertiger Grauguß und die physikalisch-metallurgischen Grundlagen seiner Herstellung影响因子(影响力)




书目名称Hochwertiger Grauguß und die physikalisch-metallurgischen Grundlagen seiner Herstellung影响因子(影响力)学科排名




书目名称Hochwertiger Grauguß und die physikalisch-metallurgischen Grundlagen seiner Herstellung网络公开度




书目名称Hochwertiger Grauguß und die physikalisch-metallurgischen Grundlagen seiner Herstellung网络公开度学科排名




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书目名称Hochwertiger Grauguß und die physikalisch-metallurgischen Grundlagen seiner Herstellung被引频次学科排名




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书目名称Hochwertiger Grauguß und die physikalisch-metallurgischen Grundlagen seiner Herstellung读者反馈学科排名

Ostrich

Eugen Piwowarsky much work germane to understanding the atomic mechanisms responsible for diffusion in semiconductors has been published. The object of the present book is to give an account of, and to consolidate, present knowledge of semiconductor diffusion in terms of basic concepts of atomic migration in crystalline latt978-1-4615-8638-8978-1-4615-8636-4

轻率看法

Eugen Piwowarskyn the band structure [1]. The varied band structures and large range of energy gaps possible with the III–V compounds have led to many potential applications. The crystal structure, lattice constant, type of energy gap, and the room temperature energy gap are summarized in Table 6.1 for the elementa

Vo2-Max

Eugen Piwowarskydependent process. Mass loss plays an important role in limiting the size of anomalies: it determines an upper effective temperature limit of about 16,000 K for the HgMn phenomenon and of about 25,000 K for helium stars. Magnetic fields can stabilize the outer convection zones leading to Ap stars wi

Free-Radical

Eugen Piwowarskyhe importance of a competing process. The effects of both mass loss and turbulence have been calculated in detail and are described. It is found that both processes have similar effects on surface abundances. The abundance anomalies on AmFm stars can be reasonably well represented by including eithe

seroma

Eugen Piwowarskyhe importance of a competing process. The effects of both mass loss and turbulence have been calculated in detail and are described. It is found that both processes have similar effects on surface abundances. The abundance anomalies on AmFm stars can be reasonably well represented by including eithe

得意牛

窒息

Nucleate

并入

Eugen Piwowarskyhe real-time imaging of the nanoscale organization of cell walls, the quantification of subcellular chemical heterogeneities, the mapping and functional analysis of individual cell wall constituents, and the probing of the nanomechanical properties of living bacteria. It is expected that in the near