Le tabagisme chez les écoliers en Valais: 2002-2010

Introduction: Le tabagisme est une cause majeure de maladies et de décès dans la population en Valais. Près d'un valaisan sur trois et une valaisanne sur quatre sont fumeurs. L'initiation au tabagisme a lieu le plus souvent à l'adolescence. Il est dès lors important de connaître les habitudes tabagiques des écoliers valaisans. Méthodes: Tous les quatre ans, le Valais et les autres cantons suisses participent à l'enquête Health Behaviour in School aged Chidren (HBSC), qui est réalisée dans plus de 40 pays sous l'égide de l'Organisation mondiale de la santé. L'objectif est de récolter et d'analyser des données pertinentes sur les comportements de santé des écoliers de 11 à 15 ans, et notamment sur le tabagisme. L'enquête HBSC 2010 a été menée dans 71 classes auprès de 1'198 écoliers en Valais. Les données ont été récoltées par questionnaire. Résultats: De nombreux écoliers valaisans de 11-15 ans ont déjà fumé au moins une fois dans leur vie. Alors que très peu d'écoliers sont des fumeurs quotidiens avant l'âge de 14 ans, près d'un écolier sur six (17% des garçons et des filles) affirme fumer quotidiennement à 15 ans. Entre 2002 et 2010, les proportions d'écoliers ayant fumé au moins une fois ou fumant quotidiennement ont diminué. Les écoliers de 14-15 ans fumant régulièrement (au moins une fois par semaine) rapportent avoir acheté le plus souvent eux mêmes leurs cigarettes ou se les êtres procurées auprès de connaissances. 42% des écoliers et 44% des écolières ont au moins leur mère, leur père ou un de leurs frères et soeurs qui fument. Conclusions et perspectives : Le tabagisme est fréquent dans la population valaisanne, et ce dès l'adolescence. La prévalence du tabagisme a légèrement diminué chez les écoliers entre 2002 et 2010. Toutefois, l'augmentation marquée de l'initiation tabagique entre 11 et 15 ans et la prévalence importante des fumeurs quotidiens parmi les écoliers de 15 ans confirment que la prévention du tabagisme est nécessaire dès le plus jeune âge. L'accessibilité des écoliers au tabac devrait être évaluée et des mesures devraient être renforcées pour la diminuer

Instabilities of a liquid layer locally heated on its free surface

International audienceWe report experimental results concerning patterns in a model experiment built to studybuoyant-thermocapillary-driven flows. The fluid is situated in a cooled cylindrical container andlocally heated on its free surface. The resulting temperature gradient induces a basic flow whichdraws the surface fluid from the hot center toward the cold boundary. When the gradient is increasedand depending on the height of liquid, the basic flow destabilizes into different stationary patterns.Above a second threshold, the patterns become time-dependent. These different instabilities arecharacterized and compared to recent theoretical results

HCOOCH3 as a probe of temperature and structure of Orion-KL

We studied the O-bearing molecule HCOOCH3 to characterize the physical conditions of the different molecular source components in Orion-KL. We identify 28 methyl formate emission peaks throughout the 50" field of observations. The two strongest peaks are in the Compact Ridge (MF1) and in the SouthWest of the Hot Core (MF2). Spectral confusion is still prevailing as half of the expected transitions are blended over the region. Assuming that the transitions are thermalized, we derive the temperature at the five main emission peaks. At the MF1 position we find a temperature of 80K in a 1.8"x0.8" beam size and 120K on a larger scale (3.6" x2.2"), suggesting an external source of heating, whereas the temperature is about 130K at the MF2 position on both scales. Transitions of HCOOCH3 in vt=1 are detected as well and the good agreement of the positions on the rotational diagrams between the vt=0 and the vt=1 transitions suggests a similar temperature. The velocity of the gas is between 7.5 and 8.0km/s depending on the positions and column density peaks vary from 1.6x10^16 to 1.6x10^17cm^-2. A second velocity component is observed around 9-10 km/s in a North-South structure stretching from the Compact Ridge up to the BN object; this component is warmer at the MF1 peak. The two other C2H4O2 isomers are not detected and the derived upper limit for the column density is <3x10^14cm^-2 for glycolaldehyde and <2x10^15cm^-2 for acetic acid. From the 223GHz continuum map, we identify several dust clumps with associated gas masses in the range 0.8 to 5.8Msun. Assuming that the HCOOCH3 is spatially distributed as the dust, we find relative abundances of HCOOCH3 in the range <0.1x10^-8 to 5.2x10^-8. We suggest a relation between the methyl formate distribution and shocks as traced by 2.12 mum H2 emission.Comment: Accepted for publication in A&

Le genre Abies en Italie: écologie générale, gestion sylvicole et ressources génétiques.

International audienceLe genre Abies est représenté en Italie par deux espèces indigènes : A. alba et A. nebrodensis. A. alba (63.400 ha) est localisé dans les Alpes et dans les Apennins, jusqu'à l'Aspromonte, en Calabre. L'article fournit d'abord un aperçu historique, puis écologique de l'utilisation des sapinières. Il décrit ensuite la gestion naturelle des ressources génétiques. Importante bibliographie

Treatment challenges in type 1 diabetes after roux-en-Y gastric bypass.

Bariatric surgery is an effective treatment of type 2 diabetes in obese patients. The obesity epidemic does not spare patients with type 1 diabetes mellitus (T1DM), but there is no consensus regarding the role of surgery in the management of obese T1DM patients. Published data consistently report significant weight loss after surgery in obese T1DM patients, but long-term glycaemic control remains difficult to achieve. Here we present our experience with a challenging patient and a review of the literature. Our patient successfully underwent a roux-en-Y gastric bypass (RYGB) when she was 28 years old. Five years after surgery, she was diagnosed with latent autoimmune diabetes of adults and insulin therapy was initiated. Insulin therapy proved very difficult to adjust, with frequent episodes of postprandial hyperglycaemia. These difficulties could only be overcome by the initiation of a subcutaneous insulin infusion using a sensor-augmented insulin pump with automated suspension. This change allowed better glycaemic control. Despite considerable weight loss with a concomitant decrease in insulin requirement, glycaemic control remained difficult after surgery. Due to their different impacts on glucose kinetics, the type of surgical operation should be part of the assessment. These patients might benefit from sensor-augmented insulin pump therapy with automated insulin suspension after bariatric surgery. The decision for surgical intervention in these patients should be carefully weighed against the difficulties in achieving adequate glycaemic control

Properties of cosmological filaments extracted from Eulerian simulations

Using a new parallel algorithm implemented within the VisIt framework, we analysed large cosmological grid simulations to study the properties of baryons in filaments. The procedure allows us to build large catalogues with up to∼3×104 filaments per simulated volume and to investigate the properties of cosmic filaments for very large volumes at high resolution (up to 3003 Mpc3 simulated with 20483 cells). We determined scaling relations for the mass, volume, length and temperature of filaments and compared them to those of galaxy clusters. The longest filaments have a total length of about 200 Mpc with a mass of several 1015 M⊙. We also investigated the effects of different gas physics. Radiative cooling significantly modifies the thermal properties of the warm-hot-intergalactic medium of filaments, mainly by lowering their mean temperature via line cooling. On the other hand, powerful feedback from active galactic nuclei in surrounding haloes can heat up the gas in filaments. The impact of shock-accelerated cosmic rays from diffusive shock acceleration on filaments is small and the ratio between cosmic ray and gas pressure within filaments is of the order of∼10-20 per cen

Dynamical structure of the inner 100 AU of the deeply embedded protostar IRAS 16293-2422

A fundamental question about the early evolution of low-mass protostars is when circumstellar disks may form. High angular resolution observations of molecular transitions in the (sub)millimeter wavelength windows make it possible to investigate the kinematics of the gas around newly-formed stars, for example to identify the presence of rotation and infall. IRAS 16293-2422 was observed with the extended Submillimeter Array (eSMA) resulting in subarcsecond resolution (0.46" x 0.29", i.e. $\sim$ 55 $\times$ 35~AU) images of compact emission from the C$^{17}$O (3-2) and C$^{34}$S (7-6) transitions at 337~GHz (0.89~mm). To recover the more extended emission we have combined the eSMA data with SMA observations of the same molecules. The emission of C$^{17}$O (3-2) and C$^{34}$S (7-6) both show a velocity gradient oriented along a northeast-southwest direction with respect to the continuum marking the location of one of the components of the binary, IRAS16293A. Our combined eSMA and SMA observations show that the velocity field on the 50--400~AU scales is consistent with a rotating structure. It cannot be explained by simple Keplerian rotation around a single point mass but rather needs to take into account the enclosed envelope mass at the radii where the observed lines are excited. We suggest that IRAS 16293-2422 could be among the best candidates to observe a pseudo-disk with future high angular resolution observations.Comment: Accepted for publication in ApJ, 18 pages, 10 figure

Theory of magnetic domains in uniaxial thin films

For uniaxial easy axis films, properties of magnetic domains are usually described within the Kittel model, which assumes that domain walls are much thinner than the domains. In this work we present a simple model that includes a proper description of the magnetostatic energy of domains and domain walls and also takes into account the interaction between both surfaces of the film. Our model describes the behavior of domain and wall widths as a function of film thickness, and is especially well suited for the strong stripe phase. We prove the existence of a critical value of magneto-crystalline anisotropy above which stripe domains exist for any film thickness and justify our model by comparison with exact results. The model is in good agreement with experimental data for hcp cobalt.Comment: 15 pages, 7 figure

Numerical simulation of fluid structure interaction in free-surface flows: the WEC case

In this work we present a numerical framework to carry-out numerical simulations of fluid-structure interaction phenomena in free-surface flows. The framework employs a singlephase method to solve momentum equations and interface advection without solving the gas phase, an immersed boundary method (IBM) to represent the moving solid within the fluid matrix and a fluid structure interaction (FSI) algorithm to couple liquid and solid phases. The method is employed to study the case of a single point wave energy converter (WEC) device, studying its free decay and its response to progressive linear waves.E.Schillaci acknowledges the financial support of the Programa Torres Quevedo (PTQ2018- 010060). The work has also been supported by a competitive R+D project (PID2020-115837RBI00) of the Spanish Research Agency.Peer ReviewedPostprint (published version