Acción colectiva rural, reforma agraria y política en El Ecuador, ca. 1920-1965

This thesis studies the rural collective action processes between 1920 and 1965 in Ecuador with a social history and political sociology approach. An approximation is carried out towards the conflicts, mobilizations and protests where indigenous and not indigenous peasants participated. Because of this, they are considered two periods, the first one that last from 1931 to 1947, sealed by the political instability and a constant change of governments; and the second one between 1948 and 1965, in a phase of successive constitutionally governments that ruled between 1948 and 1960. The conflicts and rural mobilizations reached a major visibility since 1958, deeply affecting the public opinion. The importance and magnitude of the rural mobilizations between 1959 and 1963 generated a controversy on their political effects in the agrarian change. Certainly, the rural mobilizations influenced in the outcome that took the political crisis, which concluded in the implantation of a military government in 1963. This government issued an Agrarian Reform Law in 1964, which modified partially the working relations and the land ownership. And, in addition, it defined a new type of military intervention in the policies that combined repression with reforms. The existence of a landowner social segment that backed a reform in the rural highland (sierra) society has been generally identified by Galo Plaza's figure. In his government (1948-1952), transformations were accentuated in the State intervention, mainly orientated towards the economic and political modernization. This was a new moment of coastal agro-exportation development with the leadership of the banana production. There were stimulated measures of promotion of the production and exportation of bananas. So, the road infrastructure was intensively spread and connected the producing zones with the export ports...

Mass assembly and morphological transformations since z ∼ 3 from CANDELS

We quantify the evolution of the stellar mass functions (SMFs) of star-forming and quiescent galaxies as a function of morphology from z ∼ 3 to the present. Our sample consists of ∼50 000 galaxies in the CANDELS fields (∼880 arcmin^2), which we divide into four main morphological types, i.e. pure bulge-dominated systems, pure spiral disc-dominated, intermediate two-component bulge+disc systems and irregular disturbed galaxies. At z ∼ 2, 80 per cent of the stellar mass density of star-forming galaxies is in irregular systems. However, by z ∼ 0.5, irregular objects only dominate at stellar masses below 10^9 M_⊙. A majority of the star-forming irregulars present at z ∼ 2 undergo a gradual transformation from disturbed to normal spiral disc morphologies by z ∼ 1 without significant interruption to their star formation. Rejuvenation after a quenching event does not seem to be common except perhaps for the most massive objects, because the fraction of bulge-dominated star-forming galaxies with M^*/M_⊙ > 10^10.7 reaches 40 per cent at z < 1. Quenching implies the presence of a bulge: the abundance of massive red discs is negligible at all redshifts over 2 dex in stellar mass. However, the dominant quenching mechanism evolves. At z > 2, the SMF of quiescent galaxies above M^* is dominated by compact spheroids. Quenching at this early epoch destroys the disc and produces a compact remnant unless the star-forming progenitors at even higher redshifts are significantly more dense. At 1 < z < 2, the majority of newly quenched galaxies are discs with a significant central bulge. This suggests that mass quenching at this epoch starts from the inner parts and preserves the disc. At z < 1, the high-mass end of the passive SMF is globally in place and the evolution mostly happens at stellar masses below 10^10 M_⊙. These low-mass galaxies are compact, bulge-dominated systems, which were environmentally quenched: destruction of the disc through ram-pressure stripping is the likely process.