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Artículo

Scaling relations for globular cluster systems in early-type galaxies. III : the inner flattening of the radial distributions

Caso, Juan PabloIcon ; Ennis, Ana InésIcon ; de Bórtoli, Bruno JavierIcon
Fecha de publicación: 01/2024
Editorial: Wiley Blackwell Publishing, Inc
Revista: Monthly Notices of the Royal Astronomical Society
ISSN: 0035-8711
Idioma: Inglés
Tipo de recurso: Artículo publicado
Clasificación temática:
Astronomía

Resumen

The current properties of globular cluster systems (GCSs) in the nearby Universe are a consequence of an evolutionary history ruled by accretion and disruption processes. The analysis of scaling relations for GCSs is crucial for understanding the relevance of different physical processes involved in their origin and subsequent survival. In this work, radial profiles are calculated for a sample of GCSs associated with nearby massive galaxies. This is supplemented with results from our previous papers, achieving a total sample of 53 GCSs with radial profiles homogeneously calculated, and spanning more than two orders of magnitude in stellar mass of the host galaxy. Scaling relations involving different parameters of the GCSs are obtained for the entire sample, and their significance in terms of different scenarios is considered. Finally, the results are analysed in the literature context.
Palabras clave: EARLY-TYPE GALAXIES , EVOLUTION OF GALAXIES , DARK MATTER HALOES , GLOBULAR CLUSTERS
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info:eu-repo/semantics/openAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)
Identificadores
URI: http://hdl.handle.net/11336/236559
URL: https://academic.oup.com/mnras/article/527/3/6993/7442092
DOI: http://dx.doi.org/10.1093/mnras/stad3602
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Articulos(IALP)
Articulos de INST.DE ASTROFISICA LA PLATA
Citación
Caso, Juan Pablo; Ennis, Ana Inés; de Bórtoli, Bruno Javier; Scaling relations for globular cluster systems in early-type galaxies. III : the inner flattening of the radial distributions; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 527; 3; 1-2024; 6993-7004
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