They are better able to influence their colleagues' clinical activities than a non-medical These 'doctors in the lead' bridge the medical and the management world in the hospital organization. The article examines the leadership of department heads in a university hospital in day-to-day practice. This is the first of several articles to be published in Research World on the results from ESOMAR's latest annual study on the market research sector worldwideĭoctor in the lead: balancing between two worlds The goal is to present a development of above mentioned values and to discover potential patterns and predict future trends for this tourism fair.įull Text Available The value of the total world market market research in the year 2001 was US$15,890 million, a 2.8% increase on the previous year. Data was collected in the period 2004-2008 and placed together to make a five year overview. This research focused on exhibitors', trade visitors and private visitors' origin, age distribution of private visitors, exhibiting companies, exhibiting branches, interest for travel according to type and overall impression and outlook that was gathered through surveys at ITB Berlin. Analyzed data was annually gathered by Gelzus Messe-Marktforschung GmbH. This paper analyses the key trends of this event in the last five year period (from 2004 until 2008. ITB Berlin represents the world's leading travel trade show. It is of great interest for exhibitors and visitors, as well as for host cities and organizers. ITB Berlin: The world's leading tourism fairĭirectory of Open Access Journals (Sweden)įull Text Available MICE is a significant segment of tourism industry. (Special issue with differents articles: Bid for beta beams at CERN CERN's golden jubilee Climbing the energy scale The next 20 years Working at CERN CERN and industry What's in it for British business?) (13½ pages) On the 29th September 1954 representatives of the 12 founding Mmebers States of CERN (including UK) ratified the Organisation's convention, paving the way for the establishment of one of the world's leading fundamental physics reserach institutions. Model, but additional physical effects (such as feedback and self-gravity) mustīe invoked to explain their lengths and widths.CERN celebrates 50 years of world-leading research Gradients, and Galactic plane heights ($z\approx$ 0 pc) to those in our simple Like the paradigmatic Nessie filament, have similar column densities, velocity Straighter, narrower, and denser "Bone-like" filaments, We find that observed "Giant Molecularįilaments" are consistent with being non-self-gravitating structures dominatedīy galactic dynamics. Sensitivity to projection effects and galactic environment (i.e. Physical properties of large-scale Galactic filaments, and quantify their Same analysis pipeline applied previously to observations, we analyze the Spiral-potential wells, with the latter due to differential rotation. Hypothesize that the former may be due to gas compression in the Idealized scenario, we find filaments in both the arm and interarm regions, and Projection, when viewed from the direction of our Sun in the Milky Way. Maximum approximately one filament per $\rm kpc^$ should be identified in Large-scale Galactic filaments are intrinsically rare, and we estimate that at The disk of the galaxy, we identify filaments forming purely due to galacticĭynamics, without the effects of feedback or local self-gravity. Which observed large-scale filament properties (with lengths $\gtrsim 100$ pc)Ĭan be explained by galactic dynamics alone. Simulation of a Milky Way-like galaxy, we seek to understand the extent to Download a PDF of the paper titled Synthetic Large-Scale Galactic Filaments - on their Formation, Physical Properties, and Resemblance to Observations, by Catherine Zucker and 2 other authors Download PDF Abstract: Using a population of large-scale filaments extracted from an AREPO
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