Título
On the nature of the brightest globular cluster in M81
Autor
Yalia Divakara Mayya
DANIEL ROSA GONZALEZ
MAYRA SANTIAGO CORTES
Lino Héctor Rodríguez Merino
OLGA MERCEDES VEGA CASANOVA
Luis Carrasco Bazúa
Nivel de Acceso
Acceso Abierto
Materias
Resumen o descripción
We analyse the photometric, chemical, star formation history and structural properties of the brightest globular cluster (GC) in M81, referred as GC1 in this work, with the intention of establishing its nature and origin. We find that it is a metal-rich ([Fe/H]=−0.60 ± 0.10), alpha-enhanced ([α/Fe] ~ 0.20 ± 0.05), core-collapsed (core radius rc = 1.2 pc, tidal radius rt = 76rc), old (> 13 Gyr) cluster. It has an ultraviolet excess equivalent of ~ 2500 blue horizontal branch stars. It is detected in X-rays indicative of the presence of low-mass binaries. With a mass of 1.0 × 10⁷ Mʘ, the cluster is comparable in mass to M31-G1 and is four times more massive than ω Cen. The values of rc, absolute magnitude and mean surface brightness of GC1 suggest that it could be, like massive GCs in other giant galaxies, the left-over nucleus of a dissolved dwarf galaxy.
Editor
Monthly Notices of the Royal Astronomical Society
Fecha de publicación
11 de diciembre de 2013
Tipo de publicación
Artículo
Versión de la publicación
Versión aceptada
Recurso de información
Formato
application/pdf
Idioma
Inglés
Audiencia
Estudiantes
Investigadores
Público en general
Sugerencia de citación
Mayya, Y.D., et al., (2013), On the nature of the brightest globular cluster in M81, Monthly Notices of the Royal Astronomical Society, Vol. 436(1):2763-2773
Repositorio Orígen
Repositorio Institucional del INAOE
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