Inhomogeneous molecular ring around the B[e] supergiant LHA 120-S 73

We aim to improve our knowledge on the structure and dynamics of the circumstellar disk of the LMC B[e] supergiant LHA 120-S 73. High-resolution optical and near-IR spectroscopic data were obtained over a period of 16 and 7 years, respectively. The spectra cover the diagnostic emission lines from [CaII] and [OI], as well as the CO bands. These features trace the disk at different distances from the star. We analyzed the kinematics of the individual emission regions by modeling their emission profiles. A low-resolution mid-infrared spectrum was obtained as well, which provides information on the composition of the dusty disk. All diagnostic emission features display double-peaked line profiles, which we interpret as due to Keplerian rotation. We find that LHA 120-S 73 is surrounded by at least four individual rings of material with alternating densities (or by a disk with strongly non-monotonic radial density distribution). Moreover, we find that the molecular ring must have gaps or at least strong density inhomogeneities, or in other words, a clumpy structure. The mid-infrared spectrum displays features of oxygen- and carbon-rich grain species, which indicates a long-lived, stable dusty disk. We cannot confirm the previously reported high value for the stellar rotation velocity. The line profile of HeI 5876 A is strongly variable in both width and shape and resembles of those seen in non-radially pulsating stars. A proper determination of the real underlying stellar rotation velocity is hence not possible. The existence of multiple stable and clumpy rings of alternating density recalls ring structures around planets. Although there is currently insufficient observational evidence, it is tempting to propose a scenario with one (or more) minor bodies or planets revolving around LHA 120-S 73 and stabilizing the ring system, in analogy to the shepherd moons in planetary systems.Comment: 14 pages, 13 figure, accepted for pulication in A&

On the multiplicity of the zero-age main-sequence O star Herschel 36

We present the analysis of high-resolution optical spectroscopic observations of the zero-age main-sequence O star Herschel 36 spanning six years. This star is definitely a multiple system, with at least three components detected in its spectrum. Based on our radial-velocity (RV) study, we propose a picture of a close massive binary and a more distant companion, most probably in wide orbit about each other. The orbital solution for the binary, whose components we identify as O9 V and B0.5 V, is characterized by a period of 1.5415 +/- 0.0006 days. With a spectral type O7.5 V, the third body is the most luminous component of the system and also presents RV variations with a period close to 498 days. Some possible hypotheses to explain the variability are briefly addressed and further observations are suggested.Comment: 6 pages, 2 figure

Spectral Variations of Of?p Oblique Magnetic Rotator Candidates in the Magellanic Clouds

Optical spectroscopic monitoring has been conducted of two O stars in the Small and one in the Large Magellanic Cloud, the spectral characteristics of which place them in the Of?p category, which has been established in the Galaxy to consist of oblique magnetic rotators. All of these Magellanic stars show systematic spectral variations typical of the Of?p class, further strengthening their magnetic candidacy to the point of virtual certainty. The spectral variations are related to photometric variations derived from OGLE data by Naze et al. (2015) in a parallel study, which yields rotational periods for two of them. Now circular spectropolarimetry is required to measure their fields, and ultraviolet spectroscopy to further characterize their low-metallicity, magnetically confined winds, in support of hydrodynamical analyses.Comment: 18 pages, 6 figures, accepted for publication by A

Influence of ultrasound-assisted par-frying on crust formation and browning during the production of French fries

Frying is a key processing step during the production of French fries and important for end product quality and sensory attributes. It is governed by heat and mass transfer between the frying oil and the potato strips. Crust and color of the French fries are key quality parameters and important in consumer perception. Crust formation is a result of combined heat and mass transfer effects. Convective heat transfer from frying oil to potato strips and heat conduction within the tissue cause water evaporation. Mass transfer occurs in the form of water vapor release to the frying oil and oil absorption in the outer layers of the potato strips. Browning of French fries is related to Maillard reactions between reducing sugars and amino acids. High contents of reducing sugars are often related to an undesired dark color and bitter taste of French fries. High-intensity ultrasound transmitted to liquid media causes cavitation and microstreaming, which can influence boundary layers and cell structures and result in improved heat and mass transfer. The influence of an ultrasound treatment of potato strips during the par-frying step was investigated in order to determine the effect on the resulting changes in product quality. Improved heat transfer at the product surface due to micro-streaming in the oil and a facilitated release of vapor from the product surface was observed. A faster crust formation was found at the initial phase of frying but the crust was found to become softer at longer sonication times due to persistent mechanical ultrasound effects. French fries from ultrasound assisted par-frying had a lighter color after finish-frying in comparison to the conventionally par-fried samples due to an improved release of reducing sugars from the tissue. Ultrasound-assisted par-frying showed to be effective in modifying heat and mass transfer with an impact on crust formation and browning of French fries. Further work is required regarding the optimization of parameters and sonication times

Spectral classification and properties of the O Vz stars in the Galactic O-Star Spectroscopic Survey (GOSSS)

On the basis of the Galactic O-Star Spectroscopic Survey (GOSSS), a detailed systematic investigation of the O Vz stars is presented. The currently used spectral classification criteria are rediscussed, and the Vz phenomenon is recalibrated through the addition of a quantitative criterion based on the equivalent widths of the He I 4471, He II 4542, and He II 4686 spectral lines. The GOSSS O Vz and O V populations resulting from the newly adopted spectral classification criteria are comparatively analyzed. The locations of the O Vz stars are probed, showing a concentration of the most extreme cases toward the youngest star forming regions. The occurrence of the Vz spectral peculiarity in a solar-metallicity environment, as predicted by the fastwind code, is also investigated, confirming the importance of taking into account several processes for the correct interpretation of the phenomenon.Comment: Accepted for publication in The Astronomical Journa

IGR J08408--4503: a new recurrent Supergiant Fast X-ray Transient

The supergiant fast X-ray transient IGR J08408-4503 was discovered by INTEGRAL on May 15, 2006, during a bright flare. The source shows sporadic recurrent short bright flares, reaching a peak luminosity of 10^36 erg s^-1 within less than one hour. The companion star is HD 74194, an Ob5Ib(f) supergiant star located at 3 kpc in the Vela region. We report the light curves and broad-band spectra (0.1-200 keV) of all the three flares of IGR J08408-4503 detected up to now based on INTEGRAL and Swift data. The flare spectra are well described by a power-law model with a high energy cut-off at ~15 keV. The absorption column density during the flares was found to be ~10^21 cm^-2, indicating a very low matter density around the compact object. Using the supergiant donor star parameters, the wind accretion conditions imply an orbital period of the order of one year, a spin period of the order of hours and a magnetic field of the order of 10^13 G.Comment: 5 pages, 2 figures, accepted for publication in Astrophysical Journal Letter

Varieties of capitalism and resilience clusters: an exploratory approach to European regions

Regions around the world suffered asymmetric effects with the global economic crisis of the last decade. European regions were not different, and a myriad of impacts with varied magnitudes was felt. This article, inspired by the literature of varieties of capitalism (VoC), presents statistical and econometric evidence about the differences of regional resilience, measured by the variation of economic product, unemployment and R&D across regions in European Union during the economic downturn. An exploratory approach analyses the socio‐economic resilience between different member states, and VoC ideal‐types (liberal market economies, the continental capitalism, the social‐democrat economies, the Mediterranean capitalism, and the Eastern economies). The study presents a typology of resilience clusters in European regions. There were found six types of profiles concerning resilience: great performers, fast growth, intermediate position, R&D reduction, regions in divergence, and Mediterranean regions in big trouble. The study identifies key aspects for resilience, providing policy implications for regional economic policies. The comparison of the resilience clusters and the original VoC categorization has implications for this branch of literature as it does not completely address the variety of regional answers to the shocks.info:eu-repo/semantics/acceptedVersio