Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-12-06
Astronomy and Astrophysics
Astrophysics
4 pages, accepted for publication in Astronomy & Astrophysics Letters
Scientific paper
10.1051/0004-6361:20066884
Aim: The aim is to study the stellar content of the bar region to constrain its formation and evolution. Methods: Line-strength indices in the bar region of a sample of 6 barred galaxies were employed to derive age and metallicity gradients along the bars using stellar population models. Results: We find clear radial gradients in the line-strength indices for all the galaxies. We find positive gradients within the bar region in the metal indices in four of the six galaxies, and opposite trends in the other two. These latter two galaxies are classified as SAB and they present exponential bar light profiles. For all the galaxies we find a positive gradient in the Balmer indices. There is a clear correlation between the position of morphological features inside the bar region with changes in the slope and value of the indices, which indicate, using stellar population analysis, changes in the stellar populations. Therefore, it seems that the bar regions show a gradient in both age and metallicity, changing radially to younger and more metal rich populations for all the galaxies except for those two with exponential profiles.
Perez Israel
Sanchez-Blazquez Patricia
Zurita Almudena
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