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1. |
Record Nr. |
UNINA9910827897903321 |
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Autore |
Keller Scott <1972-> |
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Titolo |
Más Allá Del Desempeño : Salud de Organización Como Máxima Ventaja Competitiva / / Scott Keller and Colin Price |
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Pubbl/distr/stampa |
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Madrid, España : , : LID Editorial Empresarial, , [2013] |
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©2013 |
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ISBN |
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Edizione |
[First edition.] |
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Descrizione fisica |
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1 online resource (1 v.) : ill |
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Collana |
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Colección Acción empresarial |
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Disciplina |
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Soggetti |
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Organizational behavior |
Organizational effectiveness |
Performance |
Corporate culture |
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Lingua di pubblicazione |
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Formato |
Materiale a stampa |
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Livello bibliografico |
Monografia |
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Note generali |
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Original title: Beyond performance, J. Wiley & Sons, 2011. Cf. Copyright page. |
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Nota di bibliografia |
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Includes bibliographical references. |
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Sommario/riassunto |
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Más allá del desempeño es una obra coral cuya filosofía es dar a conocer cuáles deben ser las prioridades de la empresa, y alcanzar un equilibrio entre el rendimiento de la empresa, el desempeño de los trabajadores y la salud corporativa de la misma. Demuestran cómo un exceso de lo uno sobre lo otro provoca una disfunción interna que acaba provocando el hundimiento de la empresa. El desempeño tiene que ver con lograr resultados económicos en el lugar y circunstancias actuales. La salud tiene que ver con la capacidad para hacerlo un año tras otro. Son dos conceptos diferentes. Algunas compañías no cuentan ni con lo uno ni con lo otro; otras, solo consiguen una de las dos cosas. Para alcanzar la máxima ventaja competitiva hay que lograr las dos. ¿Pero cómo? |
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2. |
Record Nr. |
UNINA9910437982403321 |
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Autore |
San Ramon Izaskun |
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Titolo |
The formation and evolution of M33 as revealed by its star clusters / / Izaskun San Ramon |
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Pubbl/distr/stampa |
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New York, : Springer, c2013 |
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ISBN |
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Edizione |
[1st ed. 2013.] |
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Descrizione fisica |
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1 online resource (137 p.) |
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Collana |
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Disciplina |
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Soggetti |
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Stars - Clusters |
Galaxies - Formation |
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Lingua di pubblicazione |
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Formato |
Materiale a stampa |
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Livello bibliografico |
Monografia |
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Note generali |
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Description based upon print version of record. |
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Nota di bibliografia |
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Includes bibliographical references. |
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Nota di contenuto |
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Foreword from Professor Ata Sarajedini -- Introduction -- Newly Identified Star Clusters in M33: Space-Based Survey -- Photometric Properties of the M33 Star Cluster System: Ground-Based Survey -- Structural Parameters of the M33 Star Cluster System -- Kinematic Properties of Star Clusters in M33 -- Conclusions. |
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Sommario/riassunto |
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This thesis represents the first wide-field photometric and spectroscopic survey of star clusters in the nearby late-spiral galaxy M33. This system is the nearest example of a dwarf spiral galaxy, which may have a unique role in the process of galaxy formation and evolution. The cold dark matter paradigm of galaxy formation envisions large spiral galaxies, such as the Milky Way, being formed from the merger and accretion of many smaller dwarf galaxies. The role that dwarf spiral galaxies play in this process is largely unclear. One of the goals of this thesis is to use the star cluster population of M33 to study its formation and evolution from its early stages to the present. The thesis presents a new comprehensive catalog of M33 star clusters, which includes magnitudes, colors, structural parameters, and several preliminary velocity measurements. Based on an analysis of these data, the thesis concludes that, among other things, the evolution of M33 has likely been influenced by its nearby massive neighbor M31. |
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