Magnetar outbursts: an observational review

Transient outbursts from magnetars have shown to be a key property of their emission, and one of the main way to discover new sources of this class. From the discovery of the first transient event around 2003, we now count about a dozen of outbursts, which increased the number of these strongly magnetic neutron stars by a third in six years. Magnetar outbursts might involve their multi-band emission resulting in an increased activity from radio to hard X-ray, usually with a soft X-ray flux increasing by a factor of 10-1000 with respect to the quiescent level. A connected X-ray spectral evolution is also often observed, with a spectral softening during the outburst decay. The flux decay times vary a lot from source to source, ranging from a few weeks to several years, as also the decay law which can be exponential-like, a power-law or even multiple power-laws can be required to model the flux decrease. We review here on the latest observational results on the multi-band emission of magnetars, and summarize one by one all the transient events which could be studied to date from these sources.Comment: 34 pages, 6 figures. Chapter of the Springer Book ASSP 7395 "High-energy emission from pulsars and their systems", proceeding of the Sant Cugat Forum on Astrophysics (12-16 April 2010). Review updated to January 201

Pulsar-wind nebulae and magnetar outflows: observations at radio, X-ray, and gamma-ray wavelengths

We review observations of several classes of neutron-star-powered outflows: pulsar-wind nebulae (PWNe) inside shell supernova remnants (SNRs), PWNe interacting directly with interstellar medium (ISM), and magnetar-powered outflows. We describe radio, X-ray, and gamma-ray observations of PWNe, focusing first on integrated spectral-energy distributions (SEDs) and global spectral properties. High-resolution X-ray imaging of PWNe shows a bewildering array of morphologies, with jets, trails, and other structures. Several of the 23 so far identified magnetars show evidence for continuous or sporadic emission of material, sometimes associated with giant flares, and a few possible "magnetar-wind nebulae" have been recently identified.Comment: 61 pages, 44 figures (reduced in quality for size reasons). Published in Space Science Reviews, "Jets and Winds in Pulsar Wind Nebulae, Gamma-ray Bursts and Blazars: Physics of Extreme Energy Release

The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

This paper documents the 16th data release (DR16) from the Sloan Digital Sky Surveys (SDSS), the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of data from the Southern Hemisphere survey of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2); new data from APOGEE-2 North are also included. DR16 is also notable as the final data release for the main cosmological program of the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and all raw and reduced spectra from that project are released here. DR16 also includes all the data from the Time Domain Spectroscopic Survey and new data from the SPectroscopic IDentification of ERosita Survey programs, both of which were co-observed on eBOSS plates. DR16 has no new data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey (or the MaNGA Stellar Library "MaStar"). We also preview future SDSS-V operations (due to start in 2020), and summarize plans for the final SDSS-IV data release (DR17)

Pulsar Wind Nebulae with Bow Shocks: Non-thermal Radiation and Cosmic Ray Leptons

Pulsars with high spin-down power produce relativistic winds radiating a non-negligible fraction of this power over the whole electromagnetic range from radio to gamma-rays in the pulsar wind nebulae (PWNe). The rest of the power is dissipated in the interactions of the PWNe with the ambient interstellar medium (ISM). Some of the PWNe are moving relative to the ambient ISM with supersonic speeds producing bow shocks. In this case, the ultrarelativistic particles accelerated at the termination surface of the pulsar wind may undergo reacceleration in the converging flow system formed by the plasma outflowing from the wind termination shock and the plasma inflowing from the bow shock. The presence of magnetic perturbations in the flow, produced by instabilities induced by the accelerated particles themselves, is essential for the process to work. A generic outcome of this type of reacceleration is the creation of particle distributions with very hard spectra, such as are indeed required to explain the observed spectra of synchrotron radiation with photon indices Γ≲ 1.5. The presence of this hard spectral component is specific to PWNe with bow shocks (BSPWNe). The accelerated particles, mainly electrons and positrons, may end up containing a substantial fraction of the shock ram pressure. In addition, for typical ISM and pulsar parameters, the e+ released by these systems in the Galaxy are numerous enough to contribute a substantial fraction of the positrons detected as cosmic ray (CR) particles above few tens of GeV and up to several hundred GeV. The escape of ultrarelativistic particles from a BSPWN—and hence, its appearance in the far-UV and X-ray bands—is determined by the relative directions of the interstellar magnetic field, the velocity of the astrosphere and the pulsar rotation axis. In this respect we review the observed appearance and multiwavelength spectra of three different types of BSPWNe: PSR J0437-4715, the Guitar and Lighthouse nebulae, and Vela-like objects. We argue that high resolution imaging of such objects provides unique information both on pulsar winds and on the ISM. We discuss the interpretation of imaging observations in the context of the model outlined above and estimate the BSPWN contribution to the positron flux observed at the Earth

Caracterización y distribución de facies sedimentarias en la Bahía de Cartagena, Colombia

In the sedimentological analysis of 253 sediment samples from the edges and the bottom of the Cartagena bay, we identified 26 sedimentary facies. Samples were taken with Van Veen dredge for the bottom sediment Beeker multisampler and test pits for shorelines. Using the Bernard calcimeter we carried out the calcium carbonate (CaCO3) analysis in every sieved sample. Sediments were classified according to the average grain size and content of CaCO3, to define the existing sedimentary facies, where mud litoclast facies was the most representative and distributed to the north and south of the Tierra Bomba in the internal and external bay. We found that during the past 30 years the distribution of sedimentary facies has experienced significant changes: in the inner bay the content of CaCO3 has decreased and in the southwest the grain size and content of CaCO3 have decreased, as a result of the sediments contribution from Canal del Dique and present oceanographic conditions. These hydrodynamic conditions contribute to the weathering and erosion of coral formations present in the Colombian Caribbean Keywords: Sediment, Facies, Cartagena bay, Colombian Caribbean.En el análisis sedimentológico de 253 muestras de sedimentos de fondo y borde de playa de la Bahía de Cartagena, se identificaron 26 facies sedimentarias. Las muestras fueron tomadas con draga tipo Van Veen para el fondo, multimuestreador de sedimento tipo Beeker y apiques para los bordes de playa. Las muestras fueron tamizadas y se obtuvieron 15 categorías de acuerdo al tamaño de grano, posteriormente se realizó el análisis de carbonato de calcio (CaCO3) usando el calcímetro de Bernard. Los sedimentos fueron clasificados de acuerdo con el tamaño medio de grano y el contenido de CaCO3, para definir las facies sedimentarias existentes, donde la facies lodo litoclástico es la más representativa y se distribuye en la bahía interna y externa; al norte y sur de la Isla de Tierra Bomba. Se encontró que durante los últimos 30 años la distribución de las facies sedimentarias ha experimentado variaciones significativas: en la bahía interna ha disminuido el contenido de CaCO3 y al suroeste ha disminuido el tamaño de grano y el contenido de CaCO3; como resultado del creciente aporte de sedimentos del Canal de Dique y las condiciones oceanográficas presentes. Estas condiciones hidrodinámicas favorecen la meteorización y erosión de las formaciones coralinas presentes en el Caribe Colombiano. Palabras Clave: Sedimentos, Facies, Bahía de Cartagena, Caribe Colombiano &nbsp

EFEITO DO CARBARYL SOBRE O 'RUSSETING' DA MAÇÃ (MALUS DOMESTICA BORKH.), CULTIVARES 'GALA', 'FUJI' E 'GOLDEN DELICIOUS' EFFECT OF CARBARYL ON RUSSETING OF APPLE (Malus domestica Borkh.), CULTIVARS 'GALA', 'FUJI' AND 'GOLDEN DELICIOUS'

O "russeting" da maçã caracteriza-se por uma camada de cortiça formada entre as células da epiderme e que dá um aspecto de rugosidade à superfície do fruto, depreciando-o para a comercialização. O raleio de frutos é uma prática cultural bastante difundida entre os produtores de maçã. Pode ser efetuada manualmente, quimicamente ou pela associação de ambos. Dentre os produtos mais usados para raleio químico, estão o ácido naftaleno acético (ANA) e o carbaryl, um inseticida carbamato, conhecido comercialmente como Sevinâ. Há duas formulações de carbaryl no mercado brasileiro, mas não existem dados de pesquisa suficientes que permitam escolher a formulação mais adequada. Há citações de que o carbaryl pode causar "russeting" em maçãs. O objetivo deste trabalho foi testar as duas formulações de carbaryl existentes no mercado, quanto ao seu efeito sobre o "russeting" nas maçãs. Os experimentos foram conduzidos em Fraiburgo e em Caçador, Santa Catarina, Brasil. Foram avaliadas duas concentrações, 500 ppm e 1.500 ppm de carbaryl. Foram testadas duas formulações, uma em pó-molhável com 85% de i.a. e outra em suspensão concentrada com 48% de i.a. Como a incidência de "russeting" varia entre cultivares, testou-se em 'Gala', 'Fuji' e 'Golden Delicious', que são as três mais importantes no mercado brasileiro. Os resultados mostraram que: 1) A ocorrência de "russeting" para as três cultivares foi maior em Fraiburgo do que em Caçador; 2) O carbaryl, na formulação solução concentrada, causou mais "russeting" em 'Golden Delicious', em Caçador, indicando que o seu uso deve ser evitado para essa cultivar, dando-se preferência à formulação pó-molhável; 3)Tanto a formulação quanto a concentração de carbaryl não afetaram a incidência de "russeting" nas cultivares 'Gala' e 'Fuji' nos dois locais.<br>Russeting is characterized by the development of a cork layer among the epidermal cells giving an aspect of rugosity to the fruit surface, reducing its marketability. Fruit thinning is a technique widely used by apple growers. It can be done by hand or by using chemical thinning or by both, chemical and hand thinning. Among the most used chemical for thinning are naphthaleneacetic acid (NAA) and the insecticide carbaryl, commonly known as Sevinâ. In the Brazilian market there are two formulations of carbaryl: wetted powder and flowable solution. None of them are registered as chemical thinning for apple in Brazil. However there is not enough official research data in Brazil in this area that could support the best choice as far as russeting on the fruit is concerned. Some authors say that carbaryl may cause russeting on apples. This trial aimed to evaluate the two carbaryl formulations comparing its effect concerned to russeting. The experiments were carried out in two areas: Fraiburgo and Caçador, Santa Catarina State, Brazil. Two concentrations: 500 ppm and 1.500 ppm of each formulation were tested. One of the formulations was a wetted powder with 85% of a.i., the other was a flowable solution with 48% of a.i. As the incidence of russeting on apple may vary according to cultivar, the experiments were carried out on 'Gala', 'Fuji' and 'Golden Delicious'. It was concluded that: 1) Fraiburgo climactic conditions were much more favorable to russeting than those in Caçador; 2) carbaryl did not cause russeting on 'Gala' and 'Fuji' in both locations; 3) Carbaryl as flowable solution caused more russeting in 'Golden Delicious' at Caçador, so this formulation should not be recommended for this cultivar

Flying Into the Wind: Insects and Bio-Inspired Micro-Air-Vehicles With a Wing-Stroke Dihedral Steer Passively Into Wind-Gusts

Natural fliers utilize passive and active flight control strategies to cope with windy conditions. This capability makes them incredibly agile and resistant to wind gusts. Here, we study how insects achieve this, by combining Computational Fluid Dynamics (CFD) analyses of flying fruit flies with freely-flying robotic experiments. The CFD analysis shows that flying flies are partly passively stable in side-wind conditions due to their dorsal-ventral wing-beat asymmetry defined as wing-stroke dihedral. Our robotic experiments confirm that this mechanism also stabilizes free-moving flapping robots with similar asymmetric dihedral wing-beats. This shows that both animals and robots with asymmetric wing-beats are dynamically stable in sideways wind gusts. Based on these results, we developed an improved model for the aerodynamic yaw and roll torques caused by the coupling between lateral motion and the stroke dihedral. The yaw coupling passively steers an asymmetric flapping flyer into the direction of a sideways wind gust; in contrast, roll torques are only stabilizing at high air gust velocities, due to non-linear coupling effects. The combined CFD simulations, robot experiments, and stability modeling help explain why the majority of flying insects exhibit wing-beats with positive stroke dihedral and can be used to develop more stable and robust flapping-wing Micro-Air-Vehicles.Control & Simulatio

Searching a Thousand Radio Pulsars for Gamma-ray Emission

Identifying as many gamma-ray pulsars as possible in the Fermi Large Area Telescope (LAT) data helps test pulsar emission models by comparing predicted and observed properties for a large, varied sample with as little selection bias as possible. It also improves extrapolations from the observed population to estimate the contribution of unresolved pulsars to the diffuse gamma-ray emission. We use a recently developed method to determine the probability that a given gamma-ray photon comes from a known position in the sky, convolving the photon's energy with the LAT's energy-dependent point-spread function, without the need for an accurate spatial and spectral model of the gamma-ray sky around the pulsar. The method is simple and fast and, importantly, provides probabilities, or weights, for gamma-rays from pulsars too faint for phase-integrated detection. We applied the method to over a thousand pulsars for which we obtained rotation ephemerides from radio observations, and discovered gamma-ray pulsations from 16 pulsars, 12 young and 4 recycled. PSR J2208+4056 has spindown power erg s−1, about three times lower than the previous observed gamma-ray emission "deathline." PSRs J2208+4056 and J1816−0755 have radio interpulses, constraining their geometry and perhaps enhancing their gamma-ray luminosity. We discuss whether the deathline is an artifact of selection bias due to the pulsar distance