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Departamento Gestión de Conocimiento, Monitoreo y Prospección
Consultas o comentarios: productividad@anid.cl
Consultas o comentarios: productividad@anid.cl
On central black holes in ultra-compact dwarf galaxies
| Indexado |
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| DOI | 10.1051/0004-6361/201322167 | ||||
| Año | 2013 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. Central BHs as relict tracers of tidally stripped progenitor galaxies are a plausible explanation for the elevated dynamical M/L ratios of UCDs. Direct observational tests of this scenario are suggested.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Mieske, Steffen | Hombre |
ESO - Chile
European Southern Observatory Santiago - Chile Observatorio Europeo Austral - Alemania Observatorio Europeo Austral - Chile |
| 2 | Frank, M. J. | - |
Heidelberg Univ - Alemania
|
| 3 | Baumgardt, Holger | Hombre |
UNIV QUEENSLAND - Australia
University of Queensland - Australia The University of Queensland - Australia |
| 4 | Lutzgendorf, Nora | Mujer |
ESO - Alemania
Observatorio Europeo Austral - Alemania |
| 5 | Neumayer, Nadine | Mujer |
ESO - Alemania
Observatorio Europeo Austral - Alemania |
| 6 | Hilker, Michael | Hombre |
ESO - Alemania
Observatorio Europeo Austral - Alemania |
| Fuente |
|---|
| Australian Research Council |
| Deutsche Forschungsgemeinschaft |
| German Research Foundation (DFG) via Emmy Noether Grant |
| Director General Discretionary Fund |
| Agradecimiento |
|---|
| We thank the anonymous referee for useful comments which improved this paper. M. J. F. gratefully acknowledges support from the German Research Foundation (DFG) via Emmy Noether Grant Ko 4161/1, and thanks ESO for support from the Director General Discretionary Fund. H. B. acknowledges support from the Australian Research Council through Future Fellowship grant FT0991052. |
| We thank the anonymous referee for useful comments which improved this paper. M.J.F. gratefully acknowledges support from the German Research Foundation (DFG) via Emmy Noether Grant Ko 4161/1, and thanks ESO for support from the Director General Discretionary Fund. H.B. acknowledges support from the Australian Research Council through Future Fellowship grant FT0991052. |
