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Crucial aspects of the initial mass function II. The inference of total quantities from partial information on a cluster
| Indexado |
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| DOI | 10.1051/0004-6361/201220937 | ||||
| Año | 2013 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Results. We show that the value of M that would be inferred must be described as a probability distribution Phi(M)[M; m(a), N-a, Phi(N)(N)] that depends on the completeness limit of the data, m(a), the number of stars observed down to this limit, N-a, and the prior hypothesis made on the distribution of the total number of stars in clusters, Phi(N)(N).
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | CERVINO-SAAVEDRA, MIGUEL | Hombre |
CSIC - España
Inst Astrofis Canarias - España Instituto de Astrofísica de Andalucía - CSIC - España Instituto Astrofisico de Canarias - España |
| 2 | Román-Zñiga, Carlos | Hombre |
Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México |
| 3 | Bayos, Amelia | Mujer |
ESO - Chile
Max Planck Inst Astron - Alemania European Southern Observatory Santiago - Chile Max Planck Institute for Astronomy - Alemania Observatorio Europeo Austral - Chile |
| 4 | Luridiana, V. | - |
Inst Astrofis Canarias - España
ULL - España Instituto Astrofisico de Canarias - España Universidad de La Laguna - España |
| 5 | Sanchez, N. | Hombre |
UNIV COMPLUTENSE MADRID - España
Universidad Complutense de Madrid - España |
| 6 | PEREZ-JIMENEZ, ENRIQUE | Hombre |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| Fuente |
|---|
| Consejo Nacional de Ciencia y Tecnología |
| European Commission |
| Ministerio de Ciencia e Innovación |
| Ministerio de Ciencia e Innovación |
| CONACyT, Mexico |
| Marie Curie |
| MICINN (Spain) |
| Consejo Nacional de Ciencia y TecnologÃa, Paraguay |
| Marie Curie Actions of the European Commission (FP7-COFUND) |
| programs UNAM-DGAPA-PAPIIT |
| Agradecimiento |
|---|
| We acknowledge Kevin Covey for discussions of the similarities and differences of Phi<INF>N</INF>(N) and Phi<INF>M</INF>(M) and their implications in the modeling of clusters and galaxies, which have been very useful for this paper and related works. We acknowledge the suggestions of the referee, Peter Anders, which greatly improved the clarity of the paper. This work has been supported by the MICINN (Spain) through the grants AYA2007-64712, AYA2010-15081, AYA2010-15196, AYA2011-22614, AYA2011-29754-C03-01, AYA2008-06423-C03-01/ESP, AYA2010-17631, programs UNAM-DGAPA-PAPIIT IA101812 and CONACYT 152160, Mexico, and co-funded under the Marie Curie Actions of the European Commission (FP7-COFUND). |
| We acknowledge Kevin Covey for discussions of the similarities and differences of and Φ(ℳ) and their implications in the modeling of clusters and galaxies, which have been very useful for this paper and related works. We acknowledge the suggestions of the referee, Peter Anders, which greatly improved the clarity of the paper. This work has been supported by the MICINN (Spain) through the grants AYA2007-64712, AYA2010-15081, AYA2010-15196, AYA2011-22614, AYA2011-29754-C03-01, AYA2008-06423-C03-01/ESP, AYA2010-17631, programs UNAM-DGAPA-PAPIIT IA101812 and CONACYT 152160, Mexico, and co-funded under the Marie Curie Actions of the European Commission (FP7-COFUND) ℳ |
