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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Alma Mater Studiorum - Università di Bologna
2009
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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 |
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language |
en |
format |
Doctoral Thesis |
sources |
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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 |
_version_ |
1716653975292346368 |