Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes

Whether BDs form as stars through gravitational collapse ("star-like") or BDs and some very low-mass stars constitute a separate population which form alongside stars comparable to the population of planets, e.g. through circumstellar disk ("peripheral") fragmentation, is one of the key questions of the star-formation problem. For young stars in Taurus-Auriga the binary fraction is large with little dependence on primary mass above ~0.2Msun, while for BDs it is <10%. We investigate a case in which BDs in Taurus formed dominantly through peripheral fragmentation. The decline of the binary frequency in the transition region between star-like and peripheral formation is modelled. A dynamical population synthesis model is employed in which stellar binary formation is universal. Peripheral objects form separately in circumstellar disks with a distinctive initial mass function (IMF), own orbital parameter distributions for binaries and a low binary fraction. A small amount of dynamical processing of the stellar component is accounted for as appropriate for the low-density Taurus-Auriga embedded clusters. The binary fraction declines strongly between the mass-limits for star-like and peripheral formation. The location of characteristic features and the steepness depend on these mass-limits. Such a trend might be unique to low density regions hosting dynamically unprocessed binary populations. The existence of a strong decline in the binary fraction -- primary mass diagram will become verifiable in future surveys on BD and VLMS binarity in the Taurus-Auriga star forming region. It is a test of the (non-)continuity of star formation along the mass-scale, the separateness of the stellar and BD populations and the dominant formation channel for BDs and BD binaries in regions of low stellar density hosting dynamically unprocessed populations.Comment: accepted for publication in A&A, 11 pages, 4 figures, 1 tabl

MARCO CONCEPTUAL PARA INVESTIGACIONES TSUNAMIGÉNICAS: CASO LITORAL PACÍFICO COLOMBIANO

A nivel histórico, la Costa Pacífica Colombiana ha presenciado seis tsunamis en los últimos 130 años, de los cuales dos han ocasionado completa destrucción de algunos municipios y provocado víctimas humanas. El presente trabajo pretende dar las bases conceptuales necesarias para abordar investigaciones focalizadas a la caracterización de la amenaza por tsunami, verificar el estado del arte y determinar las necesidades investigativas futuras. Toda adecuada realización de investigaciones en paleo-tsunamis debe ser multi-disciplinaria, y compilar, obtener y analizar información geológica, geomorfológica, biológica, antropológica, arqueológica e histórica, lo más detallada posible. Hasta el momento en Colombia, los trabajos realizados en torno a tsunamis han estado enfocados a la cuantificación de la inundación en localidades como Tumaco y Buenaventura. No obstante, a lo largo de la Costa Pacífica Colombiana aún no se ha trabajado en la identificación y caracterización de las fuentes de tsunami, búsqueda y caracterización de evidencias físicas de eventos pasados (e.g. depósitos de paleo-tsunamis), microzonificación sísmica regional, cambios en patrones de vegetación por eventos extremos o el impacto a la dinámica de comunidades indígenas antiguas por tsunamis, entre otros. Para que la gestión del riesgo sea efectiva, deben generarse mapas de amenaza por tsunami que integren todas las herramientas y disciplinas que identifiquen y caractericen dicha amenaza. Por ende, aquí se proponen los pasos a seguir para&nbsp;adecuadas investigaciones tsunamigénicas.Historically, the Colombian Pacific Coast has witnessed six tsunamis in the past 130 years, two of which have caused complete community destruction and human loss. The present paper aims to provide a conceptual framework needed to approach palaeo-tsunami research in the area, verifying the state of the art of tsunami hazard characterization and identifying any future investigations. Any acceptable palaeo-tsunami investigation should be multi-disciplinary, and compile, acquire and analyze in much detail, geological, geomorphological, biological, anthropological, archaeological and historical information. So far, the only research done related to tsunami hazard has been for the coastal cities of Tumaco and Buenaventura, and it has been focused on quantification of tsunami flooding. However, no research has yet been done on the identification and characterization of tsunami sources, exploration and characterization of the physical evidence of past events (e.g. palaeo-tsunami deposits), seismic micro-zonation, regional changes in vegetation patterns resulting from extreme events, or changes related to indigenous peoples’ habitational patterns or settlement abandonment, among others. For an effective risk management, tsunami hazard maps have to be emplaced, but they should integrate all the proxies and disciplines that enhance the identification and characterization of this hazard. We propose herein, the steps to follow to develop adequate tsunamigenic research

Molecular elucidation of CO2 methanation over a highly active, selective and stable LaNiO3/CeO2-derived catalyst by in situ FTIR and NAP-XPS

The CO2 methanation mechanism over the highly active (TOF=75.1 h−1), selective (>92%) and stable 10% LaNiO3/CeO2-derived catalyst is still unresolved. The surface of the catalyst is monitored under hydrogenation (H2), oxidizing (CO2) and CO2 methanation (H2 +CO2) conditions by near ambient pressure X-ray photoelectron spectroscopy (NAP-XPS) using synchrotron radiation. Meanwhile, the main reaction intermediates are identified by in situ FTIR analysis. NAP-XPS experiments confirm that LaNiO3 perovskite reduction leads to the ex-solution of Ni0 nanoparticles and Ni2+single bondCeO2−x and Ni2+single bondLa2O3 interfaces conformation, favouring the CO2 adsorption and the H2 dissociation/transfer. In situ FTIR experiments combined with the C1s spectra (NAP-XPS) suggest that the CO2 activation occurs on CeO2−x (oxygen vacancies and OH–) at low temperatures, in the form of bicarbonates; whereas, mono-/bidentate carbonates are formed on different strength La2O3 sites at increasing temperatures. These species are consecutively reduced to formates, as the main reaction intermediate, and methane by the H spilled from Ni0 nanoparticles near to NiOsingle bondCeO2−x and NiOsingle bondLa2O3 interfaces.Support for this study was provided by Projects PID2019–105960RB-C21 and PID2019–105960RB-C22 by MCIN/AEI/10.13039/501100011033, the Basque Government (Project IT1509–2022), Generalitat Valenciana (CIPROM/2021/74) and ALBA synchrotron. One of the authors (JAOC) acknowledges the postdoctoral research grant (DOCREC20/49) provided by the University of the Basque Country (UPV/EHU)

High spatial resolution optical imaging of the multiple T Tauri system LkH{\alpha} 262/LkH{\alpha} 263

We report high spatial resolution i' band imaging of the multiple T Tauri system LkH$\alpha$ 262/LkH$\alpha$ 263 obtained during the first commissioning period of the Adaptive Optics Lucky Imager (AOLI) at the 4.2 m William Herschel Telescope, using its Lucky Imaging mode. AOLI images have provided photometry for each of the two components LkH$\alpha$ 263 A and B (0.41 arcsec separation) and marginal evidence for an unresolved binary or a disc in LkH$\alpha$ 262. The AOLI data combined with previously available and newly obtained optical and infrared imaging show that the three components of LkH$\alpha$ 263 are co-moving, that there is orbital motion in the AB pair, and, remarkably, that LkH$\alpha$ 262-263 is a common proper motion system with less than 1 mas/yr relative motion. We argue that this is a likely five-component gravitationally bounded system. According to BT-settl models the mass of each of the five components is close to 0.4 M$_{\odot}$ and the age is in the range 1-2 Myr. The presence of discs in some of the components offers an interesting opportunity to investigate the formation and evolution of discs in the early stages of multiple very low-mass systems. In particular, we provide tentative evidence that the disc in 263C could be coplanar with the orbit of 263AB.Comment: 11 pages, 7 figures, Accepted 2016 May

Interaction with touchscreen smartphones in patientswith essential tremor and healthy individuals.

tremorAbstractIntroduction: Smartphone use in biomedical research is becoming more prevalent in differ-ent clinical settings. We performed a pilot study to obtain information on smartphone use bypatients with essential tremor (ET) and healthy controls, with a view to determining whetherperformance of touchscreen tasks is different between these groups and describing touchscreeninteraction factors.Method: A total of 31 patients with ET and 40 sex- and age-matched healthy controls com-pleted a descriptive questionnaire about the use of smartphones. Participants subsequentlyinteracted with an under-development Android application, and performed 4 tests evaluatingtypical touchscreen interaction gestures; each test was performed 5 times.Result: The type of smartphone use and touchscreen interaction were not significantly differ-ent between patients and controls. Age and frequency of smartphone use are key factors intouchscreen interaction.Conclusion: Our results support the use of smartphone touchscreens for research into ET,although further studies are required.pre-print1030 K

Effect of fluvastatin therapy of the pattern of protein expression in monocytes of patients in primary antiphospholipid syndrome

Comunicaciones a congreso

Role of the different copper species on the activity of Cu/zeolite catalysts for SCR of NOx with NH3

The SCR of NOx with NH3 has been studied by using different Cu zeolite catalysts, prepared both with ZSM5 and BETA zeolite supports by ionic exchange or by impregnation. The catalysts were characterized by ICP-AES, N2 adsorption at −196 °C, XRD, TEM, XPS and H2-TPR. The catalysts characterization confirmed the presence of different Cu(II) species on all catalyst (CuO and Cu(II) exchanged on tetrahedral and octahedral positions of the zeolites framework). Clear evidences of Cu(I) or Cu(0) species were not obtained. CuO was more abundant in high copper-content catalysts and in ZSM5 catalysts, due to its lower ionic exchange capacity, while isolated Cu(II) ions are more abundant in low copper-content catalysts and in BETA catalysts. It was concluded that CuO catalyzes the oxidation of NO to NO2, and this favors the reduction of NOx at lower temperature (the NH3-NO2 reaction is faster than the NH3-NO reaction because NO2 is much more oxidizing than NO), whereas isolated Cu(II) ions maintain high NOx conversion at high temperatures.Financial support provided by the Spanish Ministry of Economy and Competitiveness (CTQ2012-30703), the Basque Government (IT-657-13) and the UPV/EHU (UFI11/39). One of the authors (UDLT) wants to acknowledge to the Basque Government for the PhD Research Grant (BFI-2010-330)

Estudio de diferentes protocolos de restricción alimentaria sobre el desarrollo fetoplacentario en la coneja

Two feed strategies (ad libitum throughout pregnancy and restriction during the first 20 days), combined with oestrus synchronization with eCG or not in nulliparous rabbit does, were studied