Does the primordial evolution of globular clusters include a self-enrichment phase?:
Gespeichert in:
1. Verfasser: | |
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Format: | Buch |
Sprache: | English |
Veröffentlicht: |
Bruxelles
Académie Royale de Belgique
2003
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Schriftenreihe: | Mémoires de la Classe des Sciences
Collection in-8 ; Série 3, T. 19 |
Schlagworte: | |
Online-Zugang: | Inhaltsverzeichnis |
Beschreibung: | 155 S. graph. Darst. |
ISBN: | 2803101963 |
Internformat
MARC
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Datensatz im Suchindex
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adam_text | GENEVIEVE PARMENTIER DOES THE PRIMORDIAL EVOLUTION OF GLOBULAR CLUSTERS
INCLUDE A SELF-ENRICHMENT PHASE ? CLASSE DES SCIENCES ACADEMIE ROYALE DE
BELGIQUE CONTENTS PREFACE 9 ABSTRACT 13 RESUME 15 CHAPTER 1. -
INTRODUCTION 19 1.1. SALIENT FEATURES 19 1.2. CHEMICAL (IN)HOMOGENEITY
22 1.3. SUBSYSTEMS OF GCS AND FORMATION OF THE GALAXY 24 1.4. FIELD HALO
STARS : THE GLOBULAR CLUSTER CONNECTION 28 1.5. THE EASE SCENARIO 35
CHAPTER 2. - THE EASE SCENARIO 37 2.1. THE SAMPLE OF OBSERVED FIELD HALO
STARS 37 2.2. CORRELATIONS DERIVED 38 2.3. INTERPRETATION : TWO-PHASES
GC EVOLUTION 39 PHASE 1 41 PHASE 2 42 CHAPTER 3. - THE SELF-ENRICHMENT
OF GALACTIC HALO GLOBULAR CLUSTERS: A CLUE TO THEIR FORMATION ? 45 3.1.
CURRENT STATE OF THE ART 46 3.2. THE SELF-ENRICHMENT SCENARIO 51 3.3.
SELF-ENRICHMENT MODEL DESCRIPTION 54 3.3.1. THE PROTO-GLOBULAR CLUSTER
CLOUDS 54 3.3.2. THE FORMATION OF THE FIRST GENERATION 55 3.3.3.
SUPERSHELL PROPAGATION 56 153 CONTENTS 3.4. LEVEL OF SELF-ENRICHMENT 58
3.4.1. DYNAMICAL CONSTRAINT 58 3.4.2. CHEMICAL CONSTRAINT 59 3.5.
DISCUSSION 62 3.5.1. THE IMF OF THE FIRST STELLAR GENERATION .... 62
3.5.2. OBSERVATIONAL CONSTRAINT: THE RGB NARROWNESS 66 3.6. SUMMARY 70
CHAPTER 4. - THE OLD HALO METALLICITY GRADIENT 71 4.1. TWO POPULATIONS
OF GALACTIC HALO GCS 72 4.1.1. HORIZONTAL BRANCH MORPHOLOGY 73 4.1.2. GC
AGES 74 4.1.3. KINEMATIC DIFFERENCES 75 4.1.4. DWARF GALAXIES ACCRETION
75 4.1.5. SPATIAL DISTRIBUTION 76 4.1.6. WHAT DOES THIS ALL MEAN 76 4.2.
THE METALLICITY GRADIENT 78 4.2.1. IMPORTANCE OF THE OH/YH DIVISION 78
4.2.2. PRESSURE PROFILE OF THE HOT PROTOGALACTIC BACKGROUND 81 4.2.3.
DISCUSSION 84 4.3. WERE GCS FORMED NEAR THEIR PERIGALACTICON ? ... 87
4.4. WHAT ABOUT EXTRAGALACTIC GCSS ? 89 4.5. CONCLUSIONS 90 CHAPTER 5. -
THE MASS-METALLICITY RELATION 91 5.1. SELF-ENRICHMENT AND A
MASS-METALLICITY RELATION . 91 5.2. COMPARISON OF THE MODEL WITH THE
OBSERVATIONS . 95 5.3. SUMMARY - CONCLUSIONS 98 CHAPTER 6. - FORMATION
OF THE SECOND STELLAR GENERATION 101 6.1. OBSERVATIONAL EVIDENCE FOR
TRIGGERED STAR FORMATION 102 6.2. ANALYTICAL TREATMENT OF SHELL
GRAVITATIONAL INSTABILITIES 103 6.2.1. MATHEMATICAL DESCRIPTION OF THE
PERTURBATION 103 6.2.2. SUPERSHELL PROPAGATION THROUGHOUT THE HOT
BACKGROUND 106 6.2.3. ONSET OF THE PERTURBATION 109 6.2.4. DEVELOPMENT
OF THE PERTURBATION ILL 154 CONTENTS 6.3. NUMERICAL TREATMENT OF THE
SHELL INSTABILITY .... 117 6.3.1. THE PHASE DIFFERENCE BETWEEN V AND A {
: A(|) 118 6.3.2. THE GLOBAL PARAMETERS : N AND P H 119 6.3.3. THE
INITIAL PERTURBED SURFACE DENSITY: 3 (T EM ) 121 6.3.4. THE INITIAL
PERTURBED VELOCITY: V(T EM ) 121 6.3.5. THE NUMBER OF FORMING CLUMPS: R
124 6.3.6. THE SHELL SOUND SPEED: CS 126 6.4. DISCUSSION 128 6.5.
CAVEATS 134 6.6. SUMMARY 134 CONCLUSIONS AND FUTURE PROSPECTS 137
PUBLICATIONS ASSOCIATED TO THIS WORK 141 REFEREED PUBLICATIONS 141
CONFERENCE PROCEEDINGS 141 BIBLIOGRAPHY 145 155
|
any_adam_object | 1 |
author | Parmentier, Geneviève 1973- |
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classification_rvk | SK 600 US 2000 |
ctrlnum | (OCoLC)53289567 (DE-599)BVBBV017643791 |
discipline | Physik Mathematik |
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id | DE-604.BV017643791 |
illustrated | Illustrated |
indexdate | 2024-07-09T19:20:17Z |
institution | BVB |
isbn | 2803101963 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-010611978 |
oclc_num | 53289567 |
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owner | DE-29 DE-12 |
owner_facet | DE-29 DE-12 |
physical | 155 S. graph. Darst. |
publishDate | 2003 |
publishDateSearch | 2003 |
publishDateSort | 2003 |
publisher | Académie Royale de Belgique |
record_format | marc |
series | Mémoires de la Classe des Sciences |
series2 | Mémoires de la Classe des Sciences : Collection in-8 |
spelling | Parmentier, Geneviève 1973- Verfasser (DE-588)173653561 aut Does the primordial evolution of globular clusters include a self-enrichment phase? Geneviève Parmentier Bruxelles Académie Royale de Belgique 2003 155 S. graph. Darst. txt rdacontent n rdamedia nc rdacarrier Mémoires de la Classe des Sciences : Collection in-8 Série 3, T. 19 Stars Evolution Stars Globular clusters Kosmologie (DE-588)4114294-9 gnd rswk-swf Kugelhaufen (DE-588)4298254-6 gnd rswk-swf Anreicherung (DE-588)4330194-0 gnd rswk-swf Kugelhaufen (DE-588)4298254-6 s Kosmologie (DE-588)4114294-9 s Anreicherung (DE-588)4330194-0 s DE-604 Mémoires de la Classe des Sciences Collection in-8 ; Série 3, T. 19 (DE-604)BV011107545 3,19 GBV Datenaustausch application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=010611978&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
spellingShingle | Parmentier, Geneviève 1973- Does the primordial evolution of globular clusters include a self-enrichment phase? Mémoires de la Classe des Sciences Stars Evolution Stars Globular clusters Kosmologie (DE-588)4114294-9 gnd Kugelhaufen (DE-588)4298254-6 gnd Anreicherung (DE-588)4330194-0 gnd |
subject_GND | (DE-588)4114294-9 (DE-588)4298254-6 (DE-588)4330194-0 |
title | Does the primordial evolution of globular clusters include a self-enrichment phase? |
title_auth | Does the primordial evolution of globular clusters include a self-enrichment phase? |
title_exact_search | Does the primordial evolution of globular clusters include a self-enrichment phase? |
title_full | Does the primordial evolution of globular clusters include a self-enrichment phase? Geneviève Parmentier |
title_fullStr | Does the primordial evolution of globular clusters include a self-enrichment phase? Geneviève Parmentier |
title_full_unstemmed | Does the primordial evolution of globular clusters include a self-enrichment phase? Geneviève Parmentier |
title_short | Does the primordial evolution of globular clusters include a self-enrichment phase? |
title_sort | does the primordial evolution of globular clusters include a self enrichment phase |
topic | Stars Evolution Stars Globular clusters Kosmologie (DE-588)4114294-9 gnd Kugelhaufen (DE-588)4298254-6 gnd Anreicherung (DE-588)4330194-0 gnd |
topic_facet | Stars Evolution Stars Globular clusters Kosmologie Kugelhaufen Anreicherung |
url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=010611978&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
volume_link | (DE-604)BV011107545 |
work_keys_str_mv | AT parmentiergenevieve doestheprimordialevolutionofglobularclustersincludeaselfenrichmentphase |