scholarly journals STUDING OF ROLL STEEL STRUCTURE FORMATION PROCESS

Author(s):  
N. A. Feoktistov ◽  
K. N. Vdovid ◽  
A. S. Savinov ◽  
E. V. Skripkin

Roll steel crystallization process, and formation process of it's microstructure during cooling are considered in this article. Presented results are received by conducting of laboratory experiments, metallographic researches of roll steel. Short review of science literature is carried out, data about alloys applied in roll production is showed in first part of the article. Moreover, problems in roll manufacture, with which industry have faced, as well arising due this science obligatoriness for making researches, are considered. Based on performed analysis, the researches' target is formulated. Methodology and equipment used during researches are short considered in second part of the article. Besides, influence of cooling speed on roll steel parameters: actual grain size, carbide phase quantity, and temperature intervals of its formation are reviewed. Quantity characteristics of roll steel microstructure have determined. Data received due researches in laboratory conditions are presented graphical. Conclusions based on obtained results, as well as recommendations for further researches are given in final part of the article.

2017 ◽  
pp. 980-987 ◽  
Author(s):  
Galina Kazimirovna Elyashevich ◽  
Dmitrii Vladimirovich Novikov ◽  
Ivan Sergeevich Kuryndin ◽  
Andreja Jelen ◽  
Vili Bukošek

2016 ◽  
Vol 59 (8) ◽  
pp. 565-570 ◽  
Author(s):  
A. G. Tyagunov ◽  
V. V. V’yukhin ◽  
G. V. Tyagunov ◽  
E. E. Baryshev ◽  
Yu. N. Akshentsev

1986 ◽  
Vol 7 ◽  
pp. 481-488 ◽  
Author(s):  
Robert D. Mathieu

A young cluster or association bears the imprint of the conditions at its birth for perhaps ten million years, after which the initial conditions are lost to either dilution in the galactic field or erasure by orbital mixing and stellar encounters. In its youngest years, however, the dynamical state of the system can provide valuable information concerning the structure and energetics of the parent gas, the star-formation efficiency and the star-formation process itself. This short review discusses recent theoretical and observational progress in the study of the very youngest of stellar systems.


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