A SHRM Perspective on International Compensation and Reward Systems

We re-examine the efficacy of the SHRM perspective from the vantage point of a specific HRM system, international compensation and rewards, to gain new insights into existing conceptual models. Looking at SHRM from the ground up suggests that, to continue informing our understanding of the HRM-organizational effectiveness (OE) relationship, research will need to adopt richer theory and measures of specific HRM systems and extrapolate important contextual factors that influence relationships between OE and specific HRM systems

"BURO Case Study" In "Making the Repository Count: lessons from successful implementation"

Matt Holland and Tim Denning continue the research theme and consider the importance of IRs in support of research, focussing on three areas; how the IR fits with the university organisation; how to promote the use of the IR to end users and contributors; and how to secure long term benefits for the broadest range of stakeholders. They incorporate two case studies into the discussion, and include a description of the implementation of Bournemouth University Research Online (BURO). With contributions from Emma Crowley, BURO Manager

Toward A Model of International Compensation and Rewards: Learning From how Managers Respond to Variations in Local Host Contexts

Managers and researchers recognize that the tensions created by the interplay of globalization and national environments influence the behaviors of multinational enterprises (MNEs). In order to develop a model that is useful for understanding the effects of the global and local host environments on managerial compensation, we undertook a grounded theory building study of managers in several multinationals. We use the information gained to extend two contemporary perspectives of IHRM: national culture, and strategic alignment. We develop the idea that it is the relative degree of variation (flexibility) within the local host context that is critical to understanding managers\u27 ICRS decisions. We present a different, pragmatic experimentation view of managers\u27 ICRS decision making, which we believe offers insights into the effects of the interplay of the MNE pressures to create integrated global systems and the pressures generated within the local host environments

Iron Line Diagnostics for the GRS 1915+105 Black Hole

The properties of the broad Fe line detected in two BeppoSAX observations of the microquasar GRS 1915+105 are summarized.Comment: 4 pages, 2 figures. Proc. of the II BeppoSAX Meeting: "The Restless High-Energy Universe" (Amsterdam, May 5-8, 2003), E.P.J. van den Heuvel, J.J.M. in 't Zand, and R.A.M.J. Wijers Ed

Kinetic energy release in electron-induced decay reactions of molecular ions: C3H8+ and C3H7+

We have measured the kinetic energy release (KER) distributions for electron-induced dissociation of mass-selected molecular parent and fragment ions of propane. They are compared with distributions determined for spontaneous (metastable) dissociation. The average KER for induced dissociation of C3H8+ into C3H7+ is 13.2 +/- 1.2 meV, about 42% larger than for the spontaneous reaction. This large difference is attributed to the dramatically reduced time at which the induced reaction can be sampled. In contrast, the KER for dissociation of C3H7+ into C3H5+, which is characterized by a large reverse activation energy, is hardly affected by the experimental time scale. (C) 2000 American Institute of Physics. [S0021-9606(00)00826-6]

Cosmography: Cosmology without the Einstein equations

How much of modern cosmology is really cosmography? How much of modern cosmology is independent of the Einstein equations? (Independent of the Friedmann equations?) These questions are becoming increasingly germane -- as the models cosmologists use for the stress-energy content of the universe become increasingly baroque, it behoves us to step back a little and carefully disentangle cosmological kinematics from cosmological dynamics. The use of basic symmetry principles (such as the cosmological principle) permits us to do a considerable amount, without ever having to address the vexatious issues of just how much "dark energy", "dark matter", "quintessence", and/or "phantom matter" is needed in order to satisfy the Einstein equations. This is the sub-sector of cosmology that Weinberg refers to as "cosmography", and in this article I will explore the extent to which cosmography is sufficient for analyzing the Hubble law and so describing many of the features of the universe around us.Comment: 7 pages; uses iopart.cls setstack.sty. Based on a talk presented at ACRGR4, the 4th Australasian Conference on General Relativity and Gravitation, Monash University, Melbourne, January 2004. To appear in the proceedings, in General Relativity and Gravitatio