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HI and Galaxy Formation in Loose Groups

Models of hierarchical galaxy formation predict that large numbers of low-mass, dark matter halos remain around galaxies today. These models predict an order of magnitude more halos than observed stellar satellites in the Local Group. One possible solution to this discrepancy is that the high-velocity clouds (HVCs) around the Milky Way may be associated with the excess dark matter halos and be ...

Hi-Lite - Verification by Contract

Formal methods and testing are often considered as disjoint technologies. The Hi-Lite project wants to show that both are actually complementary. The central concept are subprogram contracts, part of the upcoming Ada 2012 standard. A contract, which consists of preand postcondition, describes the specification of a subprogram, in the same syntax as Ada expressions. These contracts can be seen e...

Introduction of hi- index

The hi-index proposed by Batista et al. in 2006 is one of the complementary indicators of the h-index based on the role and status of authors. In this article, we will introduce this indicator and its features.

Changing sag mill liners type from Hi-Low to Hi-Hi at Sarcheshmeh copper complex based on physical and numerical modeling

Liner design has become an increasingly more important tool for the AG/SAG mill performance optimization. The Sarcheshmeh copper complex concentration plant uses a SAG mill lined with 48 rows of Hi-Low type liners. Because of breakage of Low type liners and cold welding, the liner replacement task of Low with new Hi type liners has become very difficult and time-consuming. With the objective of...