The 17 min orbital period in the Ultra Compact X-ray Binary 4U 0513-40

The ultracompact low-mass X-ray binary 4U 0513-40 in the globular cluster NGC1851 exhibits large amplitude X-ray flux variations with spectral changes from low/hard to high/soft states which have not been reported previously in other ultracompact X-ray binaries. Using BeppoSAX, CHANDRA and XMM Newton archival data together with recent INTEGRAL observations, we reveal a clear sinusoidal periodic signal with a period of ~17 minutes when the source is in a typical high/soft state with a dominant soft thermal component. The periodicity disappears when the source is in a low/hard state and the thermal soft component is not required any more to model the data. These properties indicate the orbital nature of the detected signal and imply an high inclination angle of the binary system (>80{\deg}).Comment: accepted MNRAS 201

Real time localization of Gamma Ray Bursts with INTEGRAL

The INTEGRAL satellite has been successfully launched in October 2002 and has recently started its operational phase. The INTEGRAL Burst Alert System (IBAS) will distribute in real time the coordinates of the GRBs detected with INTEGRAL. After a brief introduction on the INTEGRAL instruments, we describe the main IBAS characteristics and report on the initial results. During the initial performance and verification phase of the INTEGRAL mission, which lasted about two months, two GRBs have been localized with accuracy of about 2-4 arcmin. These observations have allowed us to validate the IBAS software, which is now expected to provide quick (few seconds delay) and precise (few arcmin) localization for about 10-15 GRBs per year.Comment: 6 pages, latex, 3 figures, submitted to Adv. Sp. Res., Proceedings of the 34th COSPAR Scientific Assembly, Houston, 10-19 October 200

Swift/XRT- NuSTAR spectra of type 1 AGN]{Swift/XRT- NuSTAR spectra of type 1 AGN: confirming INTEGRAL results on the high energy cut-off

We present the 0.5 - 78 keV spectral analysis of 18 broad line AGN belonging to the INTEGRAL complete sample. Using simultaneous Swift-XRT and NuSTAR observations and employing a simple phenomenological model to fit the data, we measure with a good constraint the high energy cut-off in 13 sources, while we place lower limits on 5 objects. We found a mean high-energy cut-off of 111 keV (standard deviation = 45 keV) for the whole sample, in perfect agreement with what found in our previous work using non simultaneous observations and with what recently published using NuSTAR data. This work suggests that simultaneity of the observations in the soft and hard X-ray band is important but not always essential, especially if flux and spectral variability are properly accounted for. A lesser agreement is found when we compare our cut-off measurements with the ones obtained by Ricci et al. (2017) using Swift-BAT high energy data, finding that their values are systematically higher than ours. We have investigated whether a linear correlation exists between photon index and the cut-off and found a weak one, probably to be ascribed to the non perfect modelling of the soft part of the spectra, due to the poor statistical quality of the 2-10 keV X-ray data. No correlation is also found between the Eddington ratio and the cut-off, suggesting that only using high statistical quality broad-band spectra is it possible to verify the theoretical predictions and study the physical characteristics of the hot corona and its geometry.Comment: 12 pages, 11 figures, accepted for publication in Monthly Notices of the Royal Astronomical Societ

La leyenda negra continua…: la Sardegna viceregia nella narrativa sarda fra secondo Novecento e nuovo millennio

Il saggio approfondisce l’uso pubblico della leyenda negra da parte dei romanzieri sardi, che narrano avvenimenti, realmente accaduti o totalmente inventati, ambientati in Sardegna nell’età dei viceré spagnoli. Questi romanzi contribuiscono a perpetuare il mito della leyenda negra spagnola – un mito ormai totalmente distrutto dalla storiografia – e lo riutilizzano politicamente in chiave “sardista”.The article aims to focus the public use of the leyenda negra by Sardinian novelists who write about historical facts, real or invented, happened in Sardinia at the age of Spanish viceroys. The main contribution of these novels is perpetuating the story of the Spanish leyenda negra – a myth totally destroyed by recent historiography – by reusing it in political language in a “sardista” point of view

X-ray spectral evolution of V404 Cygni in the initial phase of the 2015 outburst

The black hole binary GS 2023+338 exhibited an unprecedently bright outburst on June 2015. Since June 17th, the high energy instruments on board INTEGRAL detected an extremely variable emission during both bright and low luminosity phases, with dramatic variations of the hardness ratio on time scales of ~seconds. The analysis of the IBIS and SPI data reveals the presence of hard spectra in the brightest phases, compatible with thermal Comptonization with temperature kTe ~ 40 keV. The seed photons temperature is best fit by kT0 ~ 7 keV, that is too high to be compatible with blackbody emission from the disk. This result is consistent with the seed photons being provided by a different source, that we hypothesize to be a synchrotron driven component in the jet. During the brightest phase of flares, the hardness shows a complex pattern of correlation with flux, with a maximum energy released in the range 40-100 keV. The hard X-ray variability for E > 50 keV is correlated with flux variations in the softer band, showing that the overall source variability cannot originate entirely from absorption, but at least part of it is due to the central accreting source.Comment: 5 pages, 4 figures, accepted for publication in Astrophysical Journal Letter

Efectos de los atributos de la hembra de ñandú (Rhea americana) sobre la viabilidad del huevo

We conducted a study throughout a breeding season in a captive-bred population of Greater rheas (Rhea americana) to evaluate the association between egg viability and the female´s body weight and age. A total of 180 eggs laid by 15 females of three age classes (5 individuals per class) were collected, individually identified, and their morphometric traits, fertility and hatchability were registered. Egg fertility increased with female´s age but was unaffected by female weight. Hatching rate does not correlate with maternal attributes. The current paper contributes towards understanding the role of certain maternal attributes in egg viability. Our findings suggest that breeding Greater rheas in large flocks where free mating occurs, increases the expression of natural sexual behavior and enhances the productivity and welfare of the birds.Realizamos un estudio a lo largo de una temporada reproductiva en una población de Ñandú común (Rhea americana) en cautiverio, con el fin de evaluar la asociación entre la viabilidad del huevo y el peso corporal y la edad de la hembra. Se colectaron un total de 180 huevos depositados por 15 hembras de tres clases de edad (5 individuos por clase). Cada huevo se identificó y se registraron sus características morfométricas, su fertilidad y éxito de eclosión. La fertilidad de los huevos se incrementó con la edad de la hembra que lo produjo pero no fue afectado por el peso corporal de la misma. La tasa de eclosión no se correlacionó con los atributos maternos evaluados. El presente trabajo contribuye a comprender el rol de ciertos atributos maternos en la viabilidad del huevo. Nuestros hallazgos sugieren que la cría de ñandúes en grandes grupos, donde el libre apareamiento es posible, aumentaría la expresión de un comportamiento sexual natural mejorando la productividad y el bienestar de las avesFil: Lábaque, María Carla. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Investigaciones Biológicas y Tecnológicas. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Instituto de Investigaciones Biológicas y Tecnológicas; Argentina. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Diversidad Biológica y Ecológica. Cátedra de Ecología; ArgentinaFil: Martella, Monica Beatriz. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Diversidad Biológica y Ecológica. Cátedra de Ecología; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Diversidad y Ecología Animal. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas Físicas y Naturales. Instituto de Diversidad y Ecología Animal; ArgentinaFil: Bazzano, Gisela del Valle. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Diversidad y Ecología Animal. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas Físicas y Naturales. Instituto de Diversidad y Ecología Animal; ArgentinaFil: Navarro, Joaquin Luis. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Diversidad Biológica y Ecológica. Cátedra de Ecología; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Diversidad y Ecología Animal. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas Físicas y Naturales. Instituto de Diversidad y Ecología Animal; Argentin