An investigation of the structure and kinematics of the spiral galaxy NGC 6503

The spiral galaxy NGC 6503 exhibits a regular kinematical structure except for a remarkable drop of the stellar velocity dispersion values in the central region. To investigate the dynamics of the disc a theoretical framework has been described. This includes a mass decomposition of the galaxy into a family of disc/halo realizations compatible with the observed photometry and rotation curve. For this family stellar velocity dispersion values and stability parameters were calculated, showing that the more massive discs, although having larger dispersions, are less stable. However, a reliable theoretical description of the inner regions where the drop occurs cannot be given. That is why we have resorted to numerical calculations. Pure stellar 3d simulations have been performed for the family of decompositions. A clear result is that disc/dark halo mass ratios approaching those of the maximum disc limit generate a large bar structure. This is incompatible with the observed morphology of NGC 6503. For the larger radii the stellar kinematics resulting from the simulations essentially agrees with that predicted by the theory, but the central velocity dispersion drop could not be reproduced. A close inspection reveals that the central nuclear region is very small and bright. Therefore, tentatively, this nucleus was considered as an isothermal sphere and a core fitting procedure was applied. For an adopted equal mass-to-light ratio of disc and nucleus, a velocity dispersion of 21.5 km/s is predicted, in excellent agreement with the observed central value. The observed dispersion drop can thus be explained by a separate kinematically distinct galactic component.Comment: 14 pages, Latex, use mn.sty style fil

The Global Structure and Evolution of a Self-Gravitating Multi-phase Interstellar Medium in a Galactic Disk

Using high resolution, two-dimensional hydrodynamical simulations, we investigate the evolution of a self-gravitating multi-phase interstellar medium in the central kiloparsec region of a galactic disk. We find that a gravitationally and thermally unstable disk evolves, in a self-stabilizing manner, into a globally quasi-stable disk that consists of cold (T < 100 K), dense clumps and filaments surrounded by hot (T > 10^4 K), diffuse medium. The quasi-stationary, filamentary structure of the cold gas is remarkable. The hot gas, characterized by low-density holes and voids, is produced by shock heating. The shocks derive their energy from differential rotation and gravitational perturbations due to the formation of cold dense clumps. In the quasi-stable phase where cold and dense clouds are formed, the effective stability parameter, Q, has a value in the range 2-5. The dynamic range of our multi-phase calculations is 10^6 - 10^7 in both density and temperature. Phase diagrams for this turbulent medium are analyzed and discussed.Comment: 10 pages, 3 figures, ApJ Letters in press (vol. 516

Deviations from the Schmidt-Kennicutt relations during early galaxy evolution

We utilize detailed time-varying models of the coupled evolution of stars and the HI, H_2, and CO-bright H_2 gas phases in galaxy-sized numerical simulations to explore the evolution of gas-rich and/or metal-poor systems, expected to be numerous in the Early Universe. The inclusion of the CO-bright H_2 gas phase, and the realistic rendering of star formation as an H_2-regulated process (and the new feedback processes that this entails) allows the most realistic tracking of strongly evolving galaxies, and much better comparison with observations. We find that while galaxies eventually settle into states conforming to Schmidt-Kennicutt (S-K) relations, significant and systematic deviations of their star formation rates (SFRs) from the latter occur, especially pronounced and prolonged for ... ...This indicates potentially serious limitations of (S-K)-type relations as reliable sub-grid elements of star formation physics in simulations of structure formation in the Early Universe. We anticipate that galaxies with marked deviations from the S-K relations will be found at high redshifts as unbiased inventories of total gas mass become possible with ALMA and the EVLA.Comment: 13 pages, 3 figures, accepted for publication in the Astrophysical Journa

Relationship of care staff attitudes with social well-being and challenging behavior of nursing home residents with dementia: a cross sectional study

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'Brussel' op afstand? Een verkenning naar mogelijkheden voor maatschappelijke diensten en ruimte voor zelfsturing bij agrarisch natuurbeheer in de Europese context

De landbouw speelt een belangrijke rol bij het in stand houden en ontwikkelen van een aantrekkelijk cultuurlandschap en de biodiversiteit in de Noordelijke Friese Wouden. Het behoud van deze waarden steunt op de inzet en de vele activiteiten van de Vereniging Noordelijke Friese Wouden, op de status van Nationaal Landschap en op een aantal subsidieregelingen vanuit de overheid. Voor het aanbrengen en beheren van landschapselementen kunnen agrariërs een vergoeding van de overheid krijgen. Dit project richt zich specifiek op zelfsturingarrangementen die gericht zijn op agrarisch natuur- en landschapsbeheer. Het verkent de mogelijkheden voor de Vereniging Noordelijke Friese Wouden om meer invloed te krijgen op en verantwoordelijkheid te nemen voor het verdelen, beheren en het controleren van de besteding van de overheidsgelden voor agrarisch natuur- en landschapsbeheer. Op het huidige moment zijn deze kaders onderhevig aan discussie binnen de Europese Unie. De hervorming van het Gemeenschappelijk Landbouwbeleid (GLB) - van waaruit een deel van deze vergoedingen betaald worden - en de vereenvoudiging van het GLB staan op de politieke agenda en discussies hierover zijn in volle gang

Star formation thresholds and galaxy edges: why and where

We study global star formation thresholds in the outer parts of galaxies by investigating the stability of disk galaxies embedded in dark halos. The disks are self-gravitating, contain metals and dust, and are exposed to UV radiation. We find that the critical surface density for the existence of a cold interstellar phase depends only weakly on the parameters of the model and coincides with the empirically derived surface density threshold for star formation. Furthermore, it is shown that the drop in the thermal velocity dispersion associated with the transition from the warm to the cold gas phase triggers gravitational instability on a wide range of scales. The presence of strong turbulence does not undermine this conclusion if the disk is self-gravitating. Models based on the hypothesis that the onset of thermal instability determines the star formation threshold in the outer parts of galaxies can reproduce many observations, including the threshold radii, column densities, and the sizes of stellar disks as a function of disk scale length and mass. Finally, prescriptions are given for implementing star formation thresholds in (semi-)analytic models and three-dimensional hydrodynamical simulations of galaxy formation.Comment: 16 pages, 6 figures, accepted for publication in the Astrophysical Journal. Version 2: text significantly revised (major improvements), physics unchanged. Version 3: minor correction

Verantwoording van de methodiek 'Kwalitatieve monitor Systeeminnovaties verduurzaaming landbouw'

Dit werkdocument geeft een beschrijving van een kwalitatieve monitoringsmethodiek die gebruikt is binnen het project ‘Monitor systeeminnovaties verduurzaming landbouw’. In dit project zijn drie systeeminnovaties gericht op een verduurzaming van de landbouw gemonitord namelijk: integraal duurzame stallen, gesloten voer-mest kringlopen en functionele agrobiodiversiteit. Het project is onderdeel van een omvangrijker project ‘Monitoring verduurzaming landbouw’ dat in opdracht van het ministerie van Landbouw, Natuur en Voedselkwaliteit onder regie van het Planbureau voor de Leefomgeving is uitgevoerd

On the Neutral Gas Content and Environment of NGC 3109 and the Antlia Dwarf Galaxy

As part of a continuing survey of nearby galaxies, we have mapped the neutral gas content of the low surface brightness, Magellanic-type galaxy NGC 3109 --- and its environment, including the Antlia dwarf galaxy --- at unprecedented velocity resolution and brightness sensitivity. The HI mass of NGC 3109 is measured to be (3.8 +/- 0.5) x 10^8 Msun. A substantial warp in the disk of NGC 3109 is detected in the HI emission image in the form of an extended low surface brightness feature. We report a positive detection in HI of the nearby Antlia dwarf galaxy, and measure its total neutral gas mass to be (6.8 +/- 1.4) x 10^5 Msun. We show the warp in NGC 3109 to lie at exactly the same radial velocity as the gas in the Antlia dwarf galaxy and speculate that Antlia disturbed the disk of NGC 3109 during a mild encounter ~1 Gyr in the past. HI data for a further eight galaxies detected in the background are presented.Comment: Accepted for publication in A