Prescribed fires

Fire is a natural disturbance phenomenon. Despite recognition of the importance of fire in ecosystems, fire suppression policies have been favoured, contributing to the accumulation of fuel in wildlands. Political options coupled with land abandonment, livestock reduction, plantation of monospecific species and the increasing number and length of summer droughts, as a consequence of climate change, are responsible for the occurrence of severe wildfires such as occurred in 2017 in Portugal and California. These kinds of fires have tremendous and unwanted impacts on the environment, society and the economy, including ecosystem services degradation and the loss of life (Nadal-Romero et al., 2018; Pereira et al., 2016a, Pereira et al., 2018). To tackle this problem, more investments are needed in preventive measures such as forest management techniques to reduce the amount of biomass in wildland environments. The most commonly used are mechanical thinning (e.g. clearcutting, partial cutting) and, if authorized by government bodies, prescribed fires ..

Scanning electron microscopy of the oral apparatus and buccopharyngeal cavity of Atelognathus salai larvae (Anura, Neobatrachia)

The aim of this study is to describe the horny structures of the buccal apparatus and buccopharyngeal cavity of A. salai by means ofscanning electron microscopy (SEM), and to compare them to those of the other known species of Atelognathus and related genera

The ACS Nearby Galaxy Survey Treasury VII. The NGC 4214 Starburst and the Effects of Star Formation History on Dwarf Morphology

We present deep Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2) optical observations obtained as part of the ACS Nearby Galaxy Survey Treasury (ANGST) as well as early release Wide Field Camera 3 (WFC3) ultra-violet and infrared observations of the nearby dwarf starbursting galaxy NGC 4214. Our data provide a detailed example of how covering such a broad range in wavelength provides a powerful tool for constraining the physical properties of stellar populations. The deepest data reach the ancient red clump at M_F814W -0.2. All of the optical data reach the main sequence turnoff for stars younger than ~300 Myr, and the blue He burning sequence for stars younger than 500 Myr. The full CMD-fitting analysis shows that all three fields in our data set are consistent with ~75% of the stellar mass being older than 8 Gyr, in spite of showing a wide range in star formation rates at the present day. Thus, our results suggest that the scale length of NGC 4214 has remained relatively constant for many Gyr. As previously noted by others, we also find the galaxy has recently ramped up production, consistent with its bright UV luminosity and its population of UV-bright massive stars. In the central field we find UV point sources with F336W magnitudes as bright as -9.9. These are as bright as stars with masses of at least 52-56 M_sun and ages near 4 Myr in stellar evolution models. Assuming a standard IMF, our CMD is well-fitted by an increase in star formation rate beginning 100 Myr ago. The stellar populations of this late-type dwarf are compared with those of NGC 404, an early-type dwarf that is also the most massive galaxy in its local environment. The late-type dwarf appears to have a similar high fraction of ancient stars, suggesting that these dominant galaxies may form at early epochs even if they have low total mass and very different present-day morphologies.Comment: 17 pages, 10 figures, accepted for publication in Ap

MAPPING THE EVOLUTION OF MENTAL HEALTH RESEARCH IN RELATION TO PHYSICAL ACTIVITY: PRE AND POST GLOBAL PANDEMIC PERSPECTIVES

The research highlights the significant impact of the COVID-19 pandemic on mental health, leading to stress, anxiety, and depression. Physical activity is recognized as a preventive strategy for overall well-being and a beneficial factor for mental health, reducing symptoms of depression and anxiety. The study uses a quantitative-bibliometric method based on keywords related to mental health, exercise, sport, social health, cognitive health, wellbeing, human development, and sports fan. The goal is to locate possible future directionalities and fields of study yet to be discovered and to study the evolution of scientific research on mental health in the social sciences in recent years. The results show that the key concepts have been evolving towards a worsening of mental health, and research linking mental health with physical activity has multiplied, particularly due to the negative effect of the readaptation to the new normality caused by the pandemic. The discussion also emphasizes the importance of social support and engagement in physical activity for mental health outcomes. The research states that group-based exercise programs and social connections are crucial for reducing symptoms of depression and anxiety. The future direction of research is also highlighted to identify effective strategies for promoting physical activity and social support during times of stress and uncertainty. Overall, understanding the relationship between physical activity and mental health can lead to improved coping skills and overall well-being

The young stellar population of NGC 4214 as observed with HST. II. Results

We present the results of a detailed UV-optical study of the nearby dwarf starburst galaxy NGC 4214 using multifilter HST/WFPC2+STIS photometry. The stellar extinction is found to be quite patchy, with some areas having values of E(4405-5495)< 0.1 mag and others, associated with star forming regions, much more heavily obscured, a result which is consistent with previous studies of the nebular extinction. We determined the ratio of blue-to-red supergiants and found it to be consistent with theoretical models for the metallicity of the SMC. The stellar IMF of the field in the range 20-100 solar masses is found to be steeper than Salpeter. A number of massive clusters and associations with ages between a few and 200 million years are detected and their properties are discussed.Comment: 49 pages, 12 figures, 6 table

Supramolecular zippers elicit interbilayer adhesion of membranes producing cell death

11 pags, 6 figsBackground: The fluorescent dye 10-N-nonyl acridine orange (NAO) is widely used as a mitochondrial marker. NAO was reported to have cytotoxic effects in cultured eukaryotic cells when incubated at high concentrations. Although the biochemical response of NAO-induced toxicity has been well identified, the underlying molecular mechanism has not yet been explored in detail. Methods: We use optical techniques, including fluorescence confocal microscopy and lifetime imaging microscopy (FLIM) both in model membranes built up as giant unilamellar vesicles (GUVs) and cultured cells. These experiments are complemented with computational studies to unravel the molecular mechanism that makes NAO cytotoxic. Results: We have obtained direct evidence that NAO promotes strong membrane adhesion of negatively charged vesicles. The attractive forces are derived from van der Waals interactions between anti-parallel H-dimers of NAO molecules from opposing bilayers. Semi-empirical calculations have confirmed the supramolecular scenario by which anti-parallel NAO molecules form a zipper of bonds at the contact region. The membrane remodeling effect of NAO, as well as the formation of H-dimers, was also confirmed in cultured fibroblasts, as shown by the ultrastructure alteration of the mitochondrial cristae. Conclusions: We conclude that membrane adhesion induced by NAO stacking accounts for the supramolecular basis of its cytotoxicity. General significance: Mitochondria are a potential target for cancer and gene therapies. The alteration of the mitochondrial structure by membrane remodeling agents able to form supramolecular assemblies via adhesion properties could be envisaged as a new therapeutic strategy.This work was supported by the ERC Starting Grant “mitochon” (ERC-StG-2013 338133) and the ERC Proof of Concept “mitozippers” (ERC-PoC-2017 780440), FIS2015-70339-C2-1-R from MINECO (I. L-M.and F.M.), FIS2015-70339-C2-2-R (M.P.L. and C.G.) and S2013/MIT-2807 from the Madrid Regional Government (F.M. and A. G-M.)

A close look at the Centaurus A group of galaxies III. Recent star formation histories of late-type dwarfs around M83

We study the resolved stellar populations of dwarf galaxies in the nearby Centaurus A/M83 group of galaxies. Our goal is to characterize their evolutionary history and to investigate eventual similarities or differences with the dwarf population in other group environments. This work presents the analysis of five late-type (irregular) dwarfs found in the vicinity of the giant spiral M83. Using archival HST/ACS data, we perform synthetic color-magnitude diagram modeling to derive the star formation histories of these late-type dwarfs. The target objects show heterogeneous star formation histories, with average star formation rates of 0.08 to 0.70x10^{-2} M_odot/yr. Some of them present prolonged, global bursts of star formation (~300-500 Myr). The studied galaxies are all metal-poor ([Fe/H] ~-1.4). We further investigate the spatial extent of different stellar populations, finding that the young stars show a clumpy distribution, as opposed to the smooth, broad extent of the old ones. The actively star forming regions have sizes of ~100 pc and lifetimes of >~100 Myr, thus suggesting a stochastic star formation mode for the target dwarf irregular galaxies. The galaxies formed ~20% to 70% of their stars more than ~7 Gyr ago. The studied dwarfs have average star formation rates slightly higher than their analogues in the Local Group, but comparable to those in the M81 group. Our preliminary sample indicates that the neutral gas content of the target dwarfs does seem to be affected by the group environment: galaxies within a denser region have a much lower M_HI/ than the isolated ones, meaning that they will exhaust their gas reservoir more quickly.Comment: 20 pages, 12 figures; accepted for publication in A&

The evolution of genomic imprinting:Theories, predictions and empirical tests

The epigenetic phenomenon of genomic imprinting has motivated the development of numerous theories for its evolutionary origins and genomic distribution. In this review, we examine the three theories that have best withstood theoretical and empirical scrutiny. These are: Haig and colleagues’ kinship theory; Day and Bonduriansky’s sexual antagonism theory; and Wolf and Hager’s maternal–offspring coadaptation theory. These theories have fundamentally different perspectives on the adaptive significance of imprinting. The kinship theory views imprinting as a mechanism to change gene dosage, with imprinting evolving because of the differential effect that gene dosage has on the fitness of matrilineal and patrilineal relatives. The sexual antagonism and maternal–offspring coadaptation theories view genomic imprinting as a mechanism to modify the resemblance of an individual to its two parents, with imprinting evolving to increase the probability of expressing the fitter of the two alleles at a locus. In an effort to stimulate further empirical work on the topic, we carefully detail the logic and assumptions of all three theories, clarify the specific predictions of each and suggest tests to discriminate between these alternative theories for why particular genes are imprinted

Factors affecting the transfer of learning to the workplace

Training aims to respond to the needs of development of individuals and organizations (Grohmann & Kauffeld, 2013). Based on Holton model, we carried out a study seeking to identify and understand the factors involved in the process of learning transfer to the workplace from two different training actions on the design and skills. The study took place at a Portuguese organization and involved 98 participants. Former students were interviewed with the purpose to explore the factors that facilitated or hindered the learning transfer, and the Inventory of the Portuguese version of the Learning Transfer System (Holton, Bates, Seyler & Carvalho, 1997; Velada & Caetano, 2009) was applied. The results suggest that the Holton model (2005) shows that the trainees have identified important issues for learning transfer and that there are differences in relation to the transfer factor pursuant to the type of training.info:eu-repo/semantics/publishedVersio