English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/170526
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:

The ALHAMBRA survey: 2D analysis of the stellar populations in massive early-type galaxies at z < 0.3

AuthorsSan Roman, I.; Cenarro, A. J.; Díaz-García, L. A.; López-Sanjuan, C.; Varela, Jesús ; González Delgado, Rosa M. ; Sánchez-Blázquez, P.; Alfaro, Emilio J. ; Ascaso, Begoña ; Bonoli, S.; Borlaff, Alejandro; Castander, Francisco J. ; Cerviño, Miguel ; Fernández-Soto, Alberto ; Márquez, Isabel ; Masegosa, Josefa ; Muniesa, D.; Pović, Mirjana; Viironen, Kerttu; Aguerri, J. A. L.; Benítez, Narciso ; Broadhurst, T.; Cabrera-Caño, Jesús; Cepa, Jordi; Cristóbal-Hornillos, David ; Infante, Leopoldo; Martínez, Vicente J.; Moles, Mariano ; Olmo, Ascensión del ; Perea, Jaime ; Prada, Francisco ; Quintana, José María
KeywordsGalaxies: evolution
Galaxies: formation
Galaxies: photometry
Galaxies: elliptical and lenticular, cD
Issue Date2018
PublisherEDP Sciences
CitationAstronomy and Astrophysics 609: 38 (2018)
AbstractWe present a technique that permits the analysis of stellar population gradients in a relatively low-cost way compared to integral field unit (IFU) surveys. We developed a technique to analyze unresolved stellar populations of spatially resolved galaxies based on photometric multi-filter surveys. This technique allows the analysis of vastly larger samples and out to larger galactic radii. We derived spatially resolved stellar population properties and radial gradients by applying a centroidal Voronoi tessellation and performing a multicolor photometry spectral energy distribution fitting. This technique has been successfully applied to a sample of 29 massive (M > 10M) early-type galaxies at z < 0.3 from the ALHAMBRA survey. We produced detailed 2D maps of stellar population properties (age, metallicity, and extinction), which allow us to identify galactic features. Radial structures were studied, and luminosity-weighted and mass-weighted gradients were derived out to 2-3.5 R. We find that the spatially resolved stellar population mass, age, and metallicity are well represented by their integrated values. We find the gradients of early-type galaxies to be on average flat in age (⇠log Age = 0.02 ± 0.06 dex/R) and negative in metallicity (⇠[Fe/H] = -0.09 ± 0.06 dex/R). Overall,the extinction gradients are flat (⇠A = -0.03 ± 0.09 mag/R) with a wide spread. These results are in agreement with previous studies that used standard long-slit spectroscopy, and with the most recent IFU studies. According to recent simulations, these results are consistent with a scenario where early-type galaxies were formed through major mergers and where their final gradients are driven by the older ages and higher metallicity of the accreted systems. We demonstrate the scientific potential of multi-filter photometry to explore the spatially resolved stellar populations of local galaxies and confirm previous spectroscopic trends from a complementary technique.
Publisher version (URL)https://doi.org/10.1051/0004-6361/201630313
Identifiersdoi: 10.1051/0004-6361/201630313
e-issn: 1432-0746
issn: 0004-6361
Appears in Collections:(IAA) Artículos
(IFT) Artículos
(IFCA) Artículos
(ICE) Artículos
Files in This Item:
File Description SizeFormat 
Alham2D0.3.pdf33,64 MBAdobe PDFThumbnail
Show full item record

Related articles:

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.