Influência da integridade dos frutos de taperebá (Spondias mombin L.) in natura na qualidade da polpa congelada.

Encontrado na região Amazônica o taperebá é um fruto amplamente consumido, em função do sabor agradável, boa composição nutricional e presença de carotenoides. A comercialização como polpa congelada é a forma de beneficiamento mais usual no Brasil. A polpa do fruto é revestida por uma casca fina, facilmente rompida por choque mecânico, o tornando muito perecível. A coleta dos frutos na Amazônica é feita de forma manual, quando maduros se desprendem das árvores (altura de 20 a 30 metros), sendo então coletados no solo ou em telas de proteção. Tal prática resulta na perda de integridade da maioria dos frutos, o que torna mais rápida a deterioração dos mesmos. Entretanto, não há registros científicos relacionando a qualidade da polpa com a integridade dos frutos. Desta forma, o objetivo do trabalho foi avaliar esta influência, realizando a caracterização físico-química, estudos de compostos bioativos e análise microbiológica. Resultados mostraram que a polpa obtida através de frutos mais íntegros apresentou maiores teores de compostos fenólicos, vitamina C, sólidos solúveis e açúcares totais, podendo indicar que os frutos batidos possivelmente sofreram ligeiro processo fermentativo. Análises microbiológicas apresentaram contagens de bactérias e bolores e leveduras superiores, além da detecção de coliformes, inclusive fecais. Tais resultados reforçam a necessidade de técnicas mais apropriadas de coleta e da prática de pasteurização para polpa, visando a qualidade do produto final

The MBHBM Project-I: measurement of the central black hole mass in spiral galaxy NGC 3504 using molecular gas kinematics

We present a dynamical mass measurement of the supermassive black hole (SMBH) in the nearby double-barred spiral galaxy NGC 3504 as part of the Measuring Black Holes in below Milky Way (M sstarf) Mass Galaxies Project. Our analysis is based on Atacama Large Millimeter/submillimeter Array cycle 5 observations of the ${}^{12}\mathrm{CO}(2-1)$ emission line. These observations probe NGC 3504's circumnuclear gas disk (CND). Our dynamical model of the CND simultaneously constrains a black hole (BH) mass of ${1.6}_{-0.4}^{+0.6}\times {10}^{7}$ M ⊙, which is consistent with the empirical BH–galaxy scaling relations and a mass-to-light ratio in the H band of 0.44 ± 0.12 (M ⊙/${L}_{\odot }$). This measurement also relies on our new estimation of the distance to the galaxy of 32.4 ± 2.1 Mpc using the surface brightness fluctuation method, which is much further than the existing distance estimates. Additionally, our observations detect a central deficit in the ${}^{12}\mathrm{CO}(2-1)$ integrated intensity map with a diameter of 6.3 pc at the putative position of the SMBH. However, we find that a dense gas tracer CS(5 − 4) peaks at the galaxy center, filling in the 12CO(2 − 1)-attenuated hole. Holes like this one are observed in other galaxies, and our observations suggest these may be caused by changing excitation conditions rather than a true absence of molecular gas around the nucleus

Bioactive CMC-Based films enriched with green coffee oil and itsresidues.

SIAN. 17 e 18 de junho de 2019. Oral. R002

Preparing for disaster: a comparative analysis of education for critical infrastructure collapse

This article explores policy approaches to educating populations for potential critical infrastructure collapse in five different countries: the UK, the US, Germany, Japan and New Zealand. ‘Critical infrastructure’ is not always easy to define, and indeed is defined slightly differently across countries – it includes entities vital to life, such as utilities (water, energy), transportation systems and communications, and may also include social and cultural infrastructure. The article is a mapping exercise of different approaches to critical infrastructure protection and preparedness education by the five countries. The exercise facilitates a comparison of the countries and enables us to identify distinctive characteristics of each country’s approach. We argue that contrary to what most scholars of security have argued, these national approaches diverge greatly, suggesting that they are shaped more by internal politics and culture than by global approaches

The MAGPI Survey: Effects of Spiral Arms on Different Tracers of the Interstellar Medium and Stellar Populations at z~0.3

Spiral structures are important drivers of the secular evolution of disc galaxies, however, the origin of spiral arms and their effects on the development of galaxies remain mysterious. In this work, we present two three-armed spiral galaxies at z~0.3 in the Middle Age Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey. Taking advantage of the high spatial resolution (~0.6'') of the Multi-Unit Spectroscopic Unit (MUSE), we investigate the two-dimensional distributions of different spectral parameters: Halpha, gas-phase metallicity, and D4000. We notice significant offsets in Halpha (~0.2 dex) as well as gas-phase metallicities (~0.05 dex) among the spiral arms, downstream and upstream of MAGPI1202197197 (SG1202). This observational signature suggests the spiral structure in SG1202 is consistent with arising from density wave theory. No azimuthal variation in Halpha or gas-phase metallicities is observed in MAGPI1204198199 (SG1204), which can be attributed to the tighter spiral arms in SG1204 than SG1202, coming with stronger mixing effects in the disc. The absence of azimuthal D4000 variation in both galaxies suggests the stars at different ages are well-mixed between the spiral arms and distributed around the disc regions. The different azimuthal distributions in Halpha and D4000 highlight the importance of time scales traced by various spectral parameters when studying 2D distributions in spiral galaxies. This work demonstrates the feasibility of constraining spiral structures by tracing interstellar medium (ISM) and stellar population at z~0.3, with a plan to expand the study to the full MAGPI survey.Comment: 15 pages, 11 figures, 2 tables, accepted for publication in MNRA