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.

Paired structures in knowledge representation.

In this position paper we propose a consistent and unifying view to all those basic knowledge representation models that are based on the existence of two somehow opposite fuzzy concepts. A number of these basic models can be found in fuzzy logic and multi-valued logic literature. Here it is claimed that it is the semantic relationship between two paired concepts what determines the emergence of different types of neutrality, namely indeterminacy, ambivalence and conflict, widely used under different frameworks (possibly under different names). It will be shown the potential relevance of paired structures, generated from two paired concepts together with their associated neutrality, all of them to be modeled as fuzzy sets. In this way, paired structures can be viewed as a standard basic model from which different models arise. This unifying view should therefore allow a deeper analysis of the relationships between several existing knowledge representation formalisms, providing a basis from which more expressive models can be later developed.

Génesis y desarrollo de las asociaciones agrícolas y de propietarios territoriales en España

Since relatively a few years ago research work regarding the genesis and evolution of agrarian organizations in our country has been carried out. Studies with a marked regional emphasis that, rarely were able to reference the true state of the associational framework during the nineteenth century, exception made of the Sociedades Económicas and of very concrete monographic studies. It is necessary to go back to the first years of the past century to find the first descriptions and working papers alluding the agrarian associational framework in Spain. On this respect, José Elías de Molins already did a study entitled La Asociación y Cooperación Agrícolas, published in the year of 1912, in which a recount of confraternities and brotherhoods verified by the Consejo de Castilla in 1770 was done. The first of modern references related to the agrarian organizations, properly speaking, corresponds to Juan Pan-Montojo in his well known work “La naissance des associations agraries en Espagne 1833-1898”, in which the consequences and changes effected in economic power structures were reflected, once the suppression of privileges linked to the land had started, as a consequence of the strengthening of liberalism in a large portion of the state’s farms. After him, came he important works of, among others, Jordi Planas and Germán Rueda. On a comparative level, the formation of agrarian societies with mobilization capacity in other European states certainly took the same amount of time to happen. Thus, the Société des Agriculteurs de France or the Société Nationale et Centrale d’Agriculture, in 1867 and 1871, respectively, came to remind the Sociedades Económicas de Amigos del País in Spain...