Por favor, use este identificador para citar o enlazar este ítem: http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1874
Spatially resolved star formation history along the disk of M82 using multi-band photometric data
Lino Héctor Rodríguez Merino
DANIEL ROSA GONZALEZ
Yalia Divakara Mayya
Acceso Abierto
Atribución-NoComercial-SinDerivadas
Galaxies: formation
Galaxies: individual (M82)
Galaxies: star clusters: general
We present results on the star formation history and extinction in the disk of M82 over spatial scales of 10ʹʹ (∼180 pc). Multi-band photometric data covering the far-ultraviolet to the near-infrared bands were fitted to a grid of synthetic spectral energy distributions. We obtained distribution functions of age and extinction for each of the 117 apertures analyzed, taking into account observational errors through Monte Carlo simulations. These distribution functions were fitted with Gaussian functions to obtain the mean ages and extinctions together with their errors. The zones analyzed include the high surface brightness complexes defined by O’Connell & Mangano. We found that these complexes share the same star formation history and extinction as the field stellar populations in the disk. There is an indication that the stellar populations are marginally older at the outer disk (450 Myr at ∼3 kpc) as compared to the inner disk (100 Myr at 0.5 kpc). For the nuclear region (radius less than 500 pc), we obtained an age of less than 10 Myr. The results obtained in this work are consistent with the idea that the 0.5–3 kpc part of the disk of M82 formed around 90% of the stellar mass in a star-forming episode that started around 450 Myr ago and lasted for about 350 Myr. We found that field stars are the major contributors to the flux over the spatial scales analyzed in this study, with the stellar cluster contribution being 7% in the nucleus and 0.7% in the disk.
The Astrophysical Journal
01-01-2011
Artículo
Inglés
Estudiantes
Investigadores
Público en general
Rodríguez Merino, L. H., Rosa González, D. and Mayya, Y. D., (2011), Spatially resolved star formation history along the disk of M82 using multi-band photometric data, The Astrophysical Journal, Vol. 726(51):1-12
ASTRONOMÍA Y ASTROFÍSICA
Versión aceptada
acceptedVersion - Versión aceptada
Aparece en las colecciones: Artículos de Astrofísica

Cargar archivos:


Fichero Tamaño Formato  
44 Rodríguez-Merino_2011_ApJ_726_51.pdf1.65 MBAdobe PDFVisualizar/Abrir