Subsystems of the Galactic halo, their structures and compositions

It is shown that general populations of globular clusters and metal-poor field stars are components at least of three subsystems occupying different volumes in the Galaxy. The thick disk and proto-disk subsystems are genetically associated with the Galaxy. The age distributions of these two subsyste...

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Main Authors: V. A. Marsakov, T. V. Borkova
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2017-03-01
Series:Odessa Astronomical Publications
Subjects:
Online Access:http://oap.onu.edu.ua/article/view/95054
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author V. A. Marsakov
T. V. Borkova
author_facet V. A. Marsakov
T. V. Borkova
author_sort V. A. Marsakov
collection DOAJ
description It is shown that general populations of globular clusters and metal-poor field stars are components at least of three subsystems occupying different volumes in the Galaxy. The thick disk and proto-disk subsystems are genetically associated with the Galaxy. The age distributions of these two subsystems do not overlap. It is argued that heavy-element enrichment and the collapse of the proto-galactic medium occurred mainly in the period between the formation of the proto-disk halo and thick disk subsystems. The largest third subsystem has no metallicity gradient, most of its objects have retrograde motion in the Galaxy, some of them have unusually low content of a-elements, and their ages are comparatively low in average, supporting the hypothesis that the objects in this subsystem had an extragalactic origin.
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spelling doaj.art-97248169e0fa4079933b09ed8c0c6cba2022-12-21T19:26:47ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-03-01150526010.18524/1810-4215.2002.15.9505495054Subsystems of the Galactic halo, their structures and compositionsV. A. Marsakov0T. V. Borkova1Space Research Department at Rostov State UniversitySpace Research Department at Rostov State UniversityIt is shown that general populations of globular clusters and metal-poor field stars are components at least of three subsystems occupying different volumes in the Galaxy. The thick disk and proto-disk subsystems are genetically associated with the Galaxy. The age distributions of these two subsystems do not overlap. It is argued that heavy-element enrichment and the collapse of the proto-galactic medium occurred mainly in the period between the formation of the proto-disk halo and thick disk subsystems. The largest third subsystem has no metallicity gradient, most of its objects have retrograde motion in the Galaxy, some of them have unusually low content of a-elements, and their ages are comparatively low in average, supporting the hypothesis that the objects in this subsystem had an extragalactic origin.http://oap.onu.edu.ua/article/view/95054globular clustersgalaxy: abundancesgalaxy: halo
spellingShingle V. A. Marsakov
T. V. Borkova
Subsystems of the Galactic halo, their structures and compositions
Odessa Astronomical Publications
globular clusters
galaxy: abundances
galaxy: halo
title Subsystems of the Galactic halo, their structures and compositions
title_full Subsystems of the Galactic halo, their structures and compositions
title_fullStr Subsystems of the Galactic halo, their structures and compositions
title_full_unstemmed Subsystems of the Galactic halo, their structures and compositions
title_short Subsystems of the Galactic halo, their structures and compositions
title_sort subsystems of the galactic halo their structures and compositions
topic globular clusters
galaxy: abundances
galaxy: halo
url http://oap.onu.edu.ua/article/view/95054
work_keys_str_mv AT vamarsakov subsystemsofthegalactichalotheirstructuresandcompositions
AT tvborkova subsystemsofthegalactichalotheirstructuresandcompositions