Suchergebnisse

El presente trabajo examina el juicio de residencia de Luis de Valdés y Rejano, gobernador de la Nueva Vizcaya, en un sentido amplio. Más allá del rigor de lo jurídicamente entonces considerado para integrar la Residen-cia, el texto explora asimismo acusaciones presentadas en San Joseph del Parral que, finalmente, quedaron fuera del juicio; acusaciones hechas por agentes de gobierno, conocedores de lo jurídicamente procedente. A la vez, visibiliza la puesta en práctica de mecanismos activados en paralelo al propio juicio, como las Canónicas Censuras. Con este estudio de caso se pretende abonar al debate en torno al entendimiento de los mecanismos de control puestos en marcha por la Monarquía Hispánica en Indias. Hacerlo haciendo énfasis en los usos políticos y rituales del juicio, en las formas de estructurar los discursos, en la importancia de los vínculos interpersonales. Se busca pues aproximarse así a la cultura política de la época Moderna: a lo entonces entendido por buen gobierno, al miedo al escándalo, al peso del honor. ; This paper examines the Trial of Residence of Luis Valdes y Rejano, governor of New Biscay, in a broad sense. Beyond the rigor of the then legally considered to integrate the Residence, the text also explores allegations made in San Joseph del Parral that ultimately left out of the trial; allegations made by government agents, aware of the legally appropriate. At the same time, it makes visible the implementation of mechanisms activated in parallel, such as the Canonical Censures. This case study is intended to contribute to the debate on the understanding of the control mechanisms put in place by the Hispanic Monarchy in the Indies. With emphasis on the political and ritual uses of the trial, the ways of structuring discourses, the importance of interpersonal relationships. It seeks as well to approach the political culture of the early modern period: what then understood by good governance, the fear of scandal, the role and value of honor.

The hosts of long duration gamma-ray bursts (GRBs) are predominantly starburst galaxies at subsolar metallicity. At redshifts z < 1, this implies that most of them are low-mass galaxies similar to the populations of blue compact dwarfs and dwarf irregulars. What triggers the massive star-formation needed for producing a GRB progenitor is still largely unknown, as are the resolved gas properties and kinematics of these galaxies and their formation history. Here we present a sample of six spatially resolved GRB hosts at z < 0.3 observed with 3D spectroscopy at high spectral resolution (R = 8000-13 000) using FLAMES/VLT. We analyzed the resolved gas kinematics of the full sample and the abundances in a subsample with strong enough emission lines. Only two galaxies show a regular disk-like rotation field, another two are dispersion-dominated, and the remaining ones have two narrow emission components associated with different parts of the galaxy but no regular rotation field, which might indicate a recent merger. All galaxies show evidence for broad components underlying the main emission peak with σ of 50-110 km s-1. This broad component is more metal-rich than the narrow components, it is blueshifted in most cases, and it follows a different velocity structure. We find a weak correlation between the star-formation rate and the width of the broad component, its flux compared to the narrow component, and the maximum outflow velocity of the gas, but we do not find any correlation with the star-formation density, metallicity or stellar mass. We hence associate this broad component with a metal-rich outflow from star-forming regions in the host. The GRB is not located in the brightest region of the host, but is always associated with some star-forming region showing a clear wind component. Our study shows the great potential of 3D spectroscopy to study the star-formation processes and history in galaxies hosting extreme transients, the need for high signal-To-noise, and the perils using unresolved or only partially resolved data for these kinds of studies. © ESO 2021. ; CT and AdUP acknowledge support from AYA2017-89384-P, CT and AdUP also from a Ramón y Cajal fellowships RyC-2012-09984 and RyC-2012-09975, LI from a Juan de la Cierva Integración fellowship IJCI-2016-30940. DAK acknowledges support from the Spanish National Research Project RTI2018-098104-J-I00 (GRBPhot). JFAF acknowledges support from the Spanish Ministerio de Ciencia, Innovación y Universidades through the grant PRE2018-086507. SDV acknowledges support from the French National Research Agency (ANR) under contract ANR-16-CE31-0003. LC is supported by YDUN grant DFF 4090-00079. Ground based observations were collected at the VLT under program 092.D-0389(A). ; With funding from the Spanish government through the Severo Ochoa Centre of Excellence accreditation SEV-2017-0709. ; Peer reviewed

In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly observed with the X-shooter spectrograph until 31/03/2017. In total, we have obtained spectroscopic observations of 103 individual GRBs observed within 48 hours of the GRB trigger. Redshifts have been measured for 97 per cent of these, covering a redshift range from 0.059 to 7.84. Based on a set of observational selection criteria that minimise biases with regards to intrinsic properties of the GRBs, the follow-up effort has been focused on producing a homogeneously selected sample of 93 afterglow spectra for GRBs discovered by the Swift satellite. We here provide a public release of all the reduced spectra, including continuum estimates and telluric absorption corrections. For completeness, we also provide reductions for the 18 late-time observations of the underlying host galaxies. We provide an assessment of the degree of completeness with respect to the parent GRB population, in terms of the X-ray properties of the bursts in the sample and find that the sample presented here is representative of the full Swift sample. We have constrained the fraction of dark bursts to be <28 per cent and confirm previous results that higher optical darkness is correlated with increased X-ray absorption. For the 42 bursts for which it is possible, we have provided a measurement of the neutral hydrogen column density, increasing the total number of published HI column density measurements by ∼33 per cent. This dataset provides a unique resource to study the ISM across cosmic time, from the local progenitor surroundings to the intervening Universe.© ESO 2019. ; JPUF, BMJ and DX acknowledge support from the ERC-StG grant EGGS-278202. The Dark Cosmology Centre was funded by the Danish National Research Foundation. This work was supported by a VILLUM FONDEN Investigator grant to JH (project number 16599). TK acknowledges support by the European Commission under the Marie Curie Intra-European Fellowship Programme in FP7. LK and JJ acknowledges support from NOVA and NWO-FAPESP grant for advanced instrumentation in astronomy. KEH and PJ acknowledge support by a Project Grant (162948-051) from The Icelandic Research Fund. AG acknowledges the financial support from the Slovenian Research Agency (research core funding No. P1-0031 and project grant No. J1-8136). CT acknowledges support from a Spanish National Research Grant of Excellence under project AYA 2014-58381-P and funding associated to a Ramon y Cajal fellowship under grant number RyC-2012-09984. AdUP acknowledges support from a Ramon y Cajal fellowship, a BBVA Foundation Grant for Researchers and Cultural Creators, and the Spanish Ministry of Economy and Competitiveness through project AYA2014-58381-P. ZC acknowledges support from the Spanish research project AYA 2014-58381-P and support from Juan de la Cierva Incorporacion fellowships IJCI-2014-21669. DAK acknowledges support from the Spanish research project AYA 2014-58381-P and support from Juan de la Cierva Incorporacion fellowships IJCI-2015-26153. RSR acknowledges AdUP's BBVA Foundation Grant for Researchers and Cultural Creators and support from ASI (Italian Space Agency) through the Contract n. 2015-046-R.0 and from European Union Horizon 2020 Programme under the AHEAD project (grant agreement n. 654215). GL is supported by a research grant (19054) from VILLUM FONDEN. SDV acknowledges the support of the French National Research Agency (ANR) under contract ANR-16-CE31-0003 BEaPro DM acknowledges support from the Instrument Center for Danish Astrophysics (IDA). ; Peer Reviewed

Phenomenology is the philosophy of our times. Through the entire twentieth century this philosophy unfolded and flourished, following stepwise the intrinsic logic and dynamism of its original project as proposed by its founder Edmund Husserl. Now its seminal ideas have been handed over to a new era. The worldwide contributors to this volume make it manifest that phenomenological inspiration knows no cultural barriers. It penetrates and invigorates not only philosophical disciplines but also most of the sectors of knowledge, transforming our way of seeing the world, our actions toward others, and our lives. Phenomenology's universal spread has, however, oftentimes diluted its original sense, even beyond recognition, and led to a weakening of its dynamics. There is at present an urgent need to retrieve the original understanding of phenomenology, to awaken its dormant forces and redirect them. This is the aim of the present book: resourcement and reinvigoration. It is meant to be not only a reference work but also a guide for research and study. To restore the authentic vision of phenomenology, we propose returning to its foundational source in Husserl's project of a `universal science', unpacking all its creative capacities. In the three parts of this work there are traced the stages of this philosophy's progressive uncovering of the grounding levels of reality: ideal structures, constitutive consciousness, the intersubjective lifeworld, and beyond. The key concepts and phases of Husserl's thought are here exfoliated. Then the thought of the movement's classical figures and of representative thinkers in succeeding generations is elucidated. Phenomenology's geographic spread is reviewed. We then proceed to the culminating work of this philosophy, to the phenomenological life engagements so vigorously advocated by Husserl, to the life-significant issues phenomenology addresses and to how it has enriched the human sciences. Lastly the phenomenological project's new horizons on the plane of life are limned, horizons with so powerful a draw that they may be said not to beckon but to summon. Here is the movement's vanguard. This collection has 71 entries. Each entry is followed by a relevant bibliography. There is a helpful Glossary of Terms and an Index of Names