The star formation history of CALIFA galaxies: Radial structures

We have studied the radial structure of the stellar mass surface density (μ∗) and stellar population age as a function of the total stellar mass and morphology for a sample of 107 galaxies from the CALIFA survey. We applied the fossil record method based on spectral synthesis techniques to recover the star formation history (SFH), resolved in space and time, in spheroidal and disk dominated galaxies with masses from 10^9 to 10^12 M_⊙. We derived the half-mass radius, and we found that galaxies are on average 15% more compact in mass than in light. The ratio of half-mass radius to half-light radius (HLR) shows a dual dependence with galaxy stellar mass; it decreases with increasing mass for disk galaxies, but is almost constant in spheroidal galaxies. In terms of integrated versus spatially resolved properties, we find that the galaxy-averaged stellar population age, stellar extinction, and μ_∗ are well represented by their values at 1 HLR. Negative radial gradients of the stellar population ages are present in most of the galaxies, supporting an inside-out formation. The larger inner (≤1 HLR) age gradients occur in the most massive (10^11 M_⊙) disk galaxies that have the most prominent bulges; shallower age gradients are obtained in spheroids of similar mass. Disk and spheroidal galaxies show negative μ∗ gradients that steepen with stellar mass. In spheroidal galaxies, μ∗ saturates at a critical value (~7 × 10^2 M_⊙/pc^2 at 1 HLR) that is independent of the galaxy mass. Thus, all the massive spheroidal galaxies have similar local μ_∗ at the same distance (in HLR units) from the nucleus. The SFH of the regions beyond 1 HLR are well correlated with their local μ_∗, and follow the same relation as the galaxy-averaged age and μ_∗; this suggests that local stellar mass surface density preserves the SFH of disks. The SFH of bulges are, however, more fundamentally related to the total stellar mass, since the radial structure of the stellar age changes with galaxy mass even though all the spheroid dominated galaxies have similar radial structure in μ_∗. Thus, galaxy mass is a more fundamental property in spheroidal systems, while the local stellar mass surface density is more important in disks.

Regionalismos léxicos y paremiológicos en la narrativa de Jorge Amado: aspectos sociolingüístico y antropológico

The work of Jorge Amado collects and processes relevant aspects of Brazilian miscegenation and allows discussion on various issues relating to the cultural productions of the country. If on the one hand the racial mixture can be seen as the result of an harmonious process, as is traditional Brazilian thought that comes from XVIII century, on the other hand it portrays the customs of Bahian society at different times, mixing the humorous tone to the optimistic view of the world. As for the miscegenation, reality of the Bahian people, as of all Brazil, can also be analyzed in their heterogeneity, for whom observes that, in the end, the crossing of economic, social and cultural boundaries have been, in many cases, quite problematic. The aim of this work is to make a journey into reality, past and present in Brazil, to understand the lexical regionalisms present in each work; it is important to understand the history of slavery, indigenous groups and the relation that the white man had with this world. All that enormous database of spoken language (a true linguistic laboratory) served and is serving to describe the Portuguese in Brazil in its regional, ethnic and social varieties. (Bagno, 2011: 104-105) I analyze here two works by Jorge Amado, Gabriela, Clove and Cinnamon: Chronicle of an Inner City and Tieta of Agreste, which constitute the corpus of this work, which will consist in detecting an extensive glossary and the collection thereof as well as paremiological regionalisms; phrases or expressions corresponding to a region and time of Brazil...