| DOI | Trouver le DOI : https://doi.org/10.1007/978-3-540-76961-3_36 |
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| Auteur | Rechercher : Van Den Bergh, Sidney1 |
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| Affiliation | - Conseil national de recherches du Canada. Institut Herzberg d'astrophysique du CNRC
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| Format | Texte, Article |
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| Conférence | Joint ESO-FONDAP Workshop on Globular Clusters, March 6-10, 2006, Concepción, Chile |
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| Sujet | globular cluster; dwarf galaxy; galaxy luminosity; luminosity distribution; luminous galaxy |
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| Résumé | The luminosity distribution of globular clusters shows a dramatic dependence on parent galaxy luminosity. Dwarf galaxies contain far more faint globulars than do luminous galaxies. This difference is significant at the 99.7% level. On the other hand the luminosity distribution of globular clusters in dwarf galaxies does not appear to depend strongly on their host’s morphological type. The dichotomy of globular cluster masses occurs at a host galaxy mass of ~ 4 × 108 M⊙, which is almost two orders of magnitude lower than the onset of the dichotomy in globular color characteristics at ~ 3 × 1010 M⊙ that was recently noted by Forbes. |
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| Date de publication | 2009 |
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| Maison d’édition | Springer |
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| Dans | |
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| Série | |
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| Langue | anglais |
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| Publications évaluées par des pairs | Oui |
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| Numéro NPARC | 23004939 |
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| Exporter la notice | Exporter en format RIS |
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| Signaler une correction | Signaler une correction (s'ouvre dans un nouvel onglet) |
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| Identificateur de l’enregistrement | cfe0efc9-b24b-44ee-84a5-d6029f7c3745 |
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| Enregistrement créé | 2019-01-22 |
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| Enregistrement modifié | 2020-04-16 |
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