A panchromatic study of stellar populations in Galactic Globular Clusters

The aim of this Thesis is to investigate (i) how common the bimodal Blue Straggler Stars (BSS) radial distribution is in stellar clusters and (ii) which are the physical processes that can produce this bimodality. We discuss possible relations between the properties of the BSS radial distribution...

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Bibliographic Details
Main Author: Dalessandro, Emanuele <1981>
Other Authors: Ferraro, Francesco Rosario
Format: Doctoral Thesis
Language:en
Published: Alma Mater Studiorum - Università di Bologna 2009
Subjects:
Online Access:http://amsdottorato.unibo.it/1730/
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spelling ndltd-unibo.it-oai-amsdottorato.cib.unibo.it-17302014-03-24T16:27:54Z A panchromatic study of stellar populations in Galactic Globular Clusters Dalessandro, Emanuele <1981> FIS/05 Astronomia e astrofisica The aim of this Thesis is to investigate (i) how common the bimodal Blue Straggler Stars (BSS) radial distribution is in stellar clusters and (ii) which are the physical processes that can produce this bimodality. We discuss possible relations between the properties of the BSS radial distribution and the dynamical state of the hosting clusters by making use of dynamical models and simulations. When relevant, we also discuss the possible links with some cluster "anomalies" and the effects of a massive object (like Imtermediate Mass Black Hole) in the cluster center. To this purpose we present the observational multiwavelength studies of the BSS populations and their radial distributions in 5 GGCs: M5, M55, M2, NGC 2419 and NGC 6388. Alma Mater Studiorum - Università di Bologna Ferraro, Francesco Rosario 2009-03-31 Doctoral Thesis PeerReviewed application/pdf en http://amsdottorato.unibo.it/1730/ info:eu-repo/semantics/openAccess
collection NDLTD
language en
format Doctoral Thesis
sources NDLTD
topic FIS/05 Astronomia e astrofisica
spellingShingle FIS/05 Astronomia e astrofisica
Dalessandro, Emanuele <1981>
A panchromatic study of stellar populations in Galactic Globular Clusters
description The aim of this Thesis is to investigate (i) how common the bimodal Blue Straggler Stars (BSS) radial distribution is in stellar clusters and (ii) which are the physical processes that can produce this bimodality. We discuss possible relations between the properties of the BSS radial distribution and the dynamical state of the hosting clusters by making use of dynamical models and simulations. When relevant, we also discuss the possible links with some cluster "anomalies" and the effects of a massive object (like Imtermediate Mass Black Hole) in the cluster center. To this purpose we present the observational multiwavelength studies of the BSS populations and their radial distributions in 5 GGCs: M5, M55, M2, NGC 2419 and NGC 6388.
author2 Ferraro, Francesco Rosario
author_facet Ferraro, Francesco Rosario
Dalessandro, Emanuele <1981>
author Dalessandro, Emanuele <1981>
author_sort Dalessandro, Emanuele <1981>
title A panchromatic study of stellar populations in Galactic Globular Clusters
title_short A panchromatic study of stellar populations in Galactic Globular Clusters
title_full A panchromatic study of stellar populations in Galactic Globular Clusters
title_fullStr A panchromatic study of stellar populations in Galactic Globular Clusters
title_full_unstemmed A panchromatic study of stellar populations in Galactic Globular Clusters
title_sort panchromatic study of stellar populations in galactic globular clusters
publisher Alma Mater Studiorum - Università di Bologna
publishDate 2009
url http://amsdottorato.unibo.it/1730/
work_keys_str_mv AT dalessandroemanuele1981 apanchromaticstudyofstellarpopulationsingalacticglobularclusters
AT dalessandroemanuele1981 panchromaticstudyofstellarpopulationsingalacticglobularclusters
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