The M4 Core Project with HST - IV. Internal Kinematics from Accurate Radial Velocities of 2771 Cluster Members

We present a detailed study of the internal kinematics of the Galactic Globular Cluster M 4 (NGC 6121), by deriving the radial velocities from 7250 spectra for 2771 stars distributed from the upper part of the Red Giant Branch down to the Main Sequence. We describe new approaches to determine the wavelength solution from day-time calibrations and to determine the radial velocity drifts that can occur between calibration and science observations when observing with the GIRAFFE spectrograph at VLT. Two techniques to determine the radial velocity are compared, after a qualitative description of their advantages with respect to other commonly used algorithm, and a new approach to remove the sky contribution from the spectra obtained with fibre-fed spectrograph and further improve the radial velocity precision is presented. The average radial velocity of the cluster is $\langle v \rangle = 71.08 \pm 0.08$ km s$^{-1}$ with an average dispersion of $\mu_{v_c} = 3.97$ km s$^{-1}$. Using the same dataset and the same statistical approach of previous analyses, 20 additional binary candidates are found, for a total of 87 candidates. A new determination of the internal radial velocity dispersion as a function of cluster distance is presented, resulting in a dispersion of $4.5$ km s$^{-1}$ within 2$^{\prime}$ from the center of cluster and steadily decreasing outward. We statistically confirm the small amplitude of the cluster rotation, as suggested in the past by several authors. This new analysis represents a significant improvement with respect to previous results in literature and provides a fundamental observational input for the modeling of the cluster dynamics.Comment: 17 pages, 17 figures. Accepted for publication in MNRAS on September 15, 201

TASTE IV. Refining ephemeris and orbital parameters for HAT-P-20b and WASP-1b

We present four new light curves of transiting exoplanets WASP-1b and HAT-P-20b, observed within the TASTE (The Asiago Search for Transit timing variations of Exoplanets) project. We re-analyzed light curves from the literature in a homogeneous way, calculating a refined ephemeris and orbital-physical parameters for both objects. WASP-1b does not show any significant Transit Timing Variation signal at the 120 s-level. As for HAT-P-20b, we detected a deviation from our re-estimated linear ephemeris that could be ascribed to the presence of a perturber or, more probably, to a previously unnoticed high level of stellar activity. The rotational period of HAT-P-20 A we obtained from archival data (P_rot ~ 14.5 days), combined with its optical variability and strong emission of CaII H&K lines, is consistent with a young stellar age (< 1 Gyr) and support the hypothesis that stellar activity may be responsible of the measured deviations of the transit times.Comment: 7 pages, 4 figures, 3 tables, accepted to Astronomische Nachrichte

Increasing the efficiency of utilization of soil and fertilizer phosphorus in the subtropical and tropical agricultural systems C

As a rule, soils of the subtropical and tropical regions, in which rainfall is not limiting, are acidic, and low in phosphorus, and, to a less extent, in other macro and micronutrients as well, such a sulfur, boron and zinc. The establishment of a permanent agricultural prac. tice therefore, demands relatively high usage of liming and phosphatic fertilization, to begin with. Several approaches, not mutually exclusive, could be used in order to increase the efficiency of utilization of soil and fertilizer phosphorus so that, goal of diminishing costs of production is reached. The use of liming materials bringing up pH to 6.0-6.5 causes the conversion of iron and aluminum phosphates to more available calcium phosphates; on the other hand, by raising calcium saturation in the exchange complex, it improves the development and operation if the root system which allows c or a higher utilization of all soil nutrients, including phosphorus, and helps of stand water deficits which may occur. The role of mycorrhizal fungi should be considered as a way of increasing soil and fertilizer P utilization, as well as the limitations thereof. Screening of and breeding for varieties with higher efficiency of uptake and utilization of soil and fertilizer phosphorus leads to a reduction in cost of inputs and to higher benefit/cost ratios. Corrective fertilization using ground rock phosphate helps to saturate the fixation power of the soil thereby reducing, as a consequence, the need for phosphorus in the maintenance fertilization. Maintenance fertilization, in which soluble phos-phatic sources are used, could be improved by several means whose performance has been proved: limimg, granula tion, placement, use of magnesium salts. Last, cost of phosphate fertilization could be further reduced, without impairing yields, through impairing yields, through changes in technology designed to obtain products better adapted to local conditions and to the availability or raw materials and energy sources.A falta de P no solo é o fator que com mais freqüência limita a produção nas condições brasileiras, particularmente a das culturas anuais. A eficiência da adubação fosfatada pode ser aumentada de diversas maneiras que às vezes são empregadas conjuntamente, a saber: 1) Calagem - aumenta o fornecimento de P do solo e diminui a conversão do P do adubo em formas de menor aproveitamento; 2) Localização diminuindo a proporção do fósforo fixado aumenta a absorção; 3) Tipo de adubo - o aproveitamento do P2O5 pode variar em função do adubo usado; 4) Espécies e variedades -o aproveitamento do fósforo na formação da colheita é influenciado pela capacidade da planta; 5) Análise do solo - as quantidades de adubo a usar são função do teor de P do solo e da relação entre custo do fertilizante e valor do produto agrícola; 6) Magnésio - a absorção do P do adubo depende do teor de Mg no solo podendo por isso ser aumentada pelo fornecimento de calcário dolomítico ou de sais solúveis de magnésio

Eficiência de fontes e doses de fósforo na alfafa e centrosema cultivadas em latossolo amarelo.

O objetivo deste trabalho foi avaliar a eficiência agronômica de fontes e doses de P na alfafa e na centrosema, cultivadas em casa de vegetação, em Latossolo Amarelo distrófico

Fontes e doses de fósforo na concentração e no conteúdo de nitrogênio e micronutrientes na alfafa e na centrosema.

O objetivo deste trabalho foi o de avaliar o efeito de fontes e doses de fósforo na concentração e o conteúdo de N, Cu, Fe, Mn e Zn na alfafa e na centrosema cultivadas em Latossolo Vermelho-Amarelo distrófico

TASTE. III. A homogeneous study of transit time variations in WASP-3b

The TASTE project is searching for low-mass planets with the Transit Timing Variation (TTV) technique, by gathering high-precision, short-cadence light curves for a selected sample of transiting exoplanets. It has been claimed that the "hot Jupiter" WASP-3b could be perturbed by a second planet. Presenting eleven new light curves (secured at the IAC80 and UDEM telescopes) and re-analyzing thirty-eight archival light curves in a homogeneous way, we show that new data do not confirm the previously claimed TTV signal. However, we bring evidence that measurements are not consistent with a constant orbital period, though no significant periodicity can be detected. Additional dynamical modeling and follow-up observations are planned to constrain the properties of the perturber or to put upper limits to it. We provide a refined ephemeris for WASP-3b and improved orbital/physical parameters. A contact eclipsing binary, serendipitously discovered among field stars, is reported here for the first time.Comment: 10 pages, 6 figures, 4 tables; accepted for publication in A&

A possibly inflated planet around the bright, young star DS Tuc A

The origin of the observed diversity of planetary system architectures is one of the main topic of the exoplanetary research. The detection of a statistically significant sample of planets around young stars allows us to study the early stages of planet formation and evolution, but only a handful of them is known so far. In this regard, a considerable contribution is expected from the NASA TESS satellite, which is now performing a survey of $\sim 85 \%$ of the sky to search for short-period transiting planets In its first month of operations, TESS found a planet candidate with an orbital period of 8.14 days around a member of the Tuc-Hor young association ($\sim$ 40 Myr), the G6V main component of the binary system DS\,Tuc. If confirmed, it would be the first transiting planet around a young star suitable for radial velocity and/or atmospheric characterization. We aim to validate the planetary nature of this companion and to measure its orbital and physical parameters. We obtain accurate planet parameters by coupling an independent reprocessing of the TESS light curve with improved stellar parameters and the dilution caused by the binary companion; we analyse high precision archival radial velocities to impose an upper limit of about 0.1 M$_{\rm Jup}$ on the planet mass; we finally rule out the presence of external companions beyond 40 au with adaptive optics images. We confirm the presence of a young, giant (${\rm R} = 0.50$ R$_{\rm Jup}$) planet having a not negligible possibility to be inflated (theoretical mass $\lesssim 20$ M$_{\oplus}$) around DS\,Tuc~A. We discuss the feasibility of mass determination, Rossiter-McLaughlin analysis and atmosphere characterization, allowed by the brightness of the star.Comment: 12 pages, 11 figures. Accepted for publication in A&

Estudos sôbre alimentação mineral do cafeeiro.: VII. Interação entre fósforo e ferro em cafeeiro (Coffe arabica L., var. Caturra KMC) cultivado em solução nutritiva

The present work was carried out in order to study: 1 - The effect of several levels of P and Fe on the chemical composition of young coffee plants (Coffea arabica L., var. Caturra, KMC); 2 - The influence of P and Fe in the up take of N, K, Ca, and Mg as revealed by the chemical analyses of coffee tissues. Five treatments with two replicates were used, namely: 1 - Control - plants grown in the solution 2 of HOAGLAND & ARNON (1950); 2 - Omission of P; 3 - 310 p. p.m. of P; 4 - Omission of Fe; 5-28 p. p.m. of Fe. The experiment was carried out in the grenhouse, the pH of the different solutions being kept between 5. 0 and 5. 5; aeration was provided to the solutions. The following conclusions wen drawn: 1 - When P was omitted from the nutrient solution, there was an increase in N, K and Fe content of the plant as compared to the levels found in control plants; 2 - Raising the P level in the substrate brought about an apparent luxury consumption of this element as well as an increase in plant Mg; 3 - High P in the nutrient solution on the other hand, decreased Fe up take but increased the K content; 4 - K content was even higher in plants corresponding to the excess Fe treatment; 5 - A very high P content was found in the roots from the excess Fe treatment, this suggesting the formation of ferric phosphate in those organs; 6 - The control plants had less Fe than those corresponding to the minus Fe treatment