The dynamic centres of infrared-dark clouds and the formation of cores

High-mass stars have an enormous influence on the evolution of the interstellar medium in galaxies, so it is important that we understand how they form. We examine the central clumps within a sample of seven infrared-dark clouds (IRDCs) with a range of masses and morphologies. We use 1-pc-scale observations from the Northern Extended Millimeter Array (NOEMA) and the IRAM 30m telescope to trace dense cores with 2.8-mm continuum, and gas kinematics in C18O, HCO+, HNC, and N2H+ (J = 1–0). We supplement our continuum sample with six IRDCs observed at 2.9 mm with the Atacama Large Millimeter/submillimeter Array (ALMA), and examine the relationships between core- and clump-scale properties. We have developed a fully automated multiple-velocity component hyperfine line-fitting code called MWYDYN which we employ to trace the dense gas kinematics in N2H+ (1–0), revealing highly complex and dynamic clump interiors. We find that parsec-scale clump mass is the most important factor driving the evolution; more massive clumps are able to concentrate more mass into their most massive cores – with a log-normally distributed efficiency of around 9 per cent – in addition to containing the most dynamic gas. Distributions of linewidths within the most massive cores are similar to the ambient gas, suggesting that they are not dynamically decoupled, but are similarly chaotic. A number of studies have previously suggested that clumps are globally collapsing; in such a scenario, the observed kinematics of clump centres would be the direct result of gravity-driven mass inflows that become ever more complex as the clumps evolve, which in turn leads to the chaotic mass growth of their core populations

Tree-ring based reconstructions of northern Patagonia precipitation since AD 1600

Long-term reconstructions (400 years) of seasonal and annual precipitation variations were developed for northern Patagonia east of the Andes using a new set of 16 tree ring-width chronologies from Austrocedrus chilensis (D.Don) Endl. Reconstructions, which capture between 41 and 50% of the precipitation variance, show that the twentieth century contains the most extreme long periods of wetness and dryness in the past 400 years. Since about AD 1910, the reconstructions are also characterized by an increase in interannual variability and one of the highest rates of extreme events within the last 400 years. A prominent oscillation on the order of 2-2.1 years in length has been identified in the reconstructions using spectral analysis. Quasi-Biennial Oscillations have been shown to be very marked in some circulation indices of the Southern Hemisphere. Although significant oscillations within the preferred frequency domain of El Nino-Southern Oscillation (ENSO) are present in the reconstructions, no clear trod consistent responses to ENSO have been observed. Correlations of reconstructions with mean sea-level pressure around South America for the interval AD 1912-1984, reveal the influence of subtropical and high-latitude features of the atmospheric circulation on precipitation variations in northern Patagonia. Droughts result from an intensification of the subtropical Pacific anticyclone off the Chilean coast and the deepness of the circum-Antarctic trough over the South Orkney-Antarctic Peninsula sector. Mean sea-level pressure reconstructions for the South Atlantic sector of the Southern Oceans were used to evaluate the temporal stability of the relationships between northern Patagonia precipitation and high-latitude climatic variations since AD 1750. The influence of high-latitude circulation on precipitation appears to be more significant during the twentieth century, which in turn may respond to an intensification of wavenumbers 3 on the mean planetary wave structure over the Southern Hemisphere. Recent increase of precipitation variability in northern Patagonia may reflect stronger interactions between middle- and high-latitude atmospheric circulation in the Southern Hemisphere during the twentieth century

Inoculação de fungos micorrízicos arbusculares em porta-enxerto de pessegueiro cv Okinawa Inoculation of arbuscular mycorrhizal fungi in peach rootstock cv Okinawa

O presente estudo teve por objetivo avaliar a influência da inoculação de fungos micorrízicos arbusculares (FMA) sobre o crescimento vegetativo, conteúdo de macronutrientes e de substâncias de reserva de plantas do porta-enxerto de pessegueiro cv Okinawa. O experimento foi realizado em telado, e o delineamento experimental utilizado foi o de blocos casualizados, com 20 plantas por parcela e quatro repetições. Foram testadas três espécies de FMA (Acaulospora sp., Glomus clarum e Glomus etunicatum) e um tratamento-testemunha, não-inoculado. A altura, o diâmetro, a área foliar, as biomassas fresca e seca, o conteúdo de macronutrientes e de substâncias de reserva foram avaliados aos 360 dias após a semeadura. Todas as plantas inoculadas com FMA apresentaram maior altura e diâmetro, quando comparadas à testemunha, sendo que Acaulospora sp. promoveu as melhores respostas. Glomus clarum e Glomus etunicatum induziram um crescimento intermediário às plantas. Os FMAs proporcionaram aumento na absorção de nitrogênio, fósforo e potássio, associados à maior altura, diâmetro do colo, área foliar, biomassa fresca e seca da parte aérea e seca das raízes, quando comparadas à testemunha. Todas as plantas inoculadas com FMA tiveram altas taxas de colonização, acima de 90%, sendo que Acaulospora sp. colonizou mais intensamente o sistema radicular das plantas.<br>The present study aimed to evaluate the influence of the arbuscular mycorrhizal fungi (AMF) inoculation on the vegetative growth, macronutrients and carbohydrate contents in rootstock plants of peach 'Okinawa'. The experiment was realized at greenhouse conditions and a randomized block design was applied, with 20 plants per plot and four repetitions. Three AMF species (Acaulospora sp., Glomus clarum e Glomus etunicatum) and non-inoculated treatment were tested. The stem height and diameter, foliage area, fresh and dry biomass, macronutrients and carbohydrate contents were evaluated 360 days after the sowing. All the AMF inoculated plants presented bigger stem height and diameter, when compared to the non-inoculated, and Acaulospora sp. rendered the best results. G. clarum and G. etunicatum induced an intermediate and similar response of the plants. AMF favored the nitrogen, phosphorus and potassium absorption, contributing to the best plant responses regarding to stem height, diameter, foliage area, fresh and dry mass of the stem and dry mass of the roots, when compared to the non-inoculated plants. All inoculated AMF plants had high colonization rate, above 90%, and Acaulospora sp. colonized the root system of the plants most intensely