2005
DOI: 10.1590/s0104-07072005000200001
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Editorial

Abstract: EditorialTexto Contexto Enferm 2005 Abr-Jun; 14(2):155-6 EDITORIALCurrently there are perceptible changes in all areas of knowledge. These changes are considered dynamic and contribute to advances within their respective professions. Of course, some of these advances affect Nursing, interfering in its configuration as a profession of care for the human being.However, this dynamic reality causes difficulties in accompanying the change process for nurses. The technological and organizational advances contribute … Show more

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Cited by 4 publications
(4 citation statements)
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“…But star over-densities do not necessarily imply the existence of physical clusters, while the opposite may also be true. Some star clusters do not produce evident over-densities relative to the density of stars in the general Galactic field (Carraro 2006).…”
Section: Cluster Fundamental Parametersmentioning
confidence: 88%
“…But star over-densities do not necessarily imply the existence of physical clusters, while the opposite may also be true. Some star clusters do not produce evident over-densities relative to the density of stars in the general Galactic field (Carraro 2006).…”
Section: Cluster Fundamental Parametersmentioning
confidence: 88%
“…As clusters evolve through dynamical effects (internally and by interactions with the Galactic tidal field), a significant fraction of the cluster stars is gradually lost to the field. Mass segregation and evaporation of low-mass members are the main effects of dynamical interactions (de la Fuente Macros 2001; Andersen & Nordström 2000;Patat & Carraro 1995;Carraro 2006). Hence, to understand cluster evolution it is necessary to study the dense central region (the core) as well as the expanded and sparse region (the halo or corona) (Pandey et al 1988;Maciejewski 2009).…”
Section: Introductionmentioning
confidence: 99%
“…Due to the dynamic evolution processes such as stellar encounters, interactions with the Galactic tidal field, etc., a significant fraction of the cluster stars are gradually lost to the field regions. The main effects of dynamical interactions are mass segregation and evaporation of low-mass members (Andersen & Nordström 2000; Patat & Carraro 1995; Carraro 2006). Studying the sparse region (the halo) along with the dense central region (the core) is therefore necessary to understand the evolution of any cluster.…”
Section: Introductionmentioning
confidence: 99%