2,732 research outputs found

    Herschel PACS and SPIRE spectroscopy of the Photodissociation Regions associated with S 106 and IRAS 23133+6050

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    Photodissociation regions (PDRs) contain a large fraction of all of the interstellar matter in galaxies. Classical examples include the boundaries between ionized regions and molecular clouds in regions of massive star formation, marking the point where all of the photons energetic enough to ionize hydrogen have been absorbed. In this paper we determine the physical properties of the PDRs associated with the star forming regions IRAS 23133+6050 and S 106 and present them in the context of other Galactic PDRs associated with massive star forming regions. We employ Herschel PACS and SPIRE spectroscopic observations to construct a full 55-650 {\mu}m spectrum of each object from which we measure the PDR cooling lines, other fine- structure lines, CO lines and the total far-infrared flux. These measurements are then compared to standard PDR models. Subsequently detailed numerical PDR models are compared to these predictions, yielding additional insights into the dominant thermal processes in the PDRs and their structures. We find that the PDRs of each object are very similar, and can be characterized by a two-phase PDR model with a very dense, highly UV irradiated phase (n \sim 10^6 cm^(-3), G0_0 \sim 10^5) interspersed within a lower density, weaker radiation field phase (n \sim 10^4 cm^(-3), G0_0 \sim 10^4). We employed two different numerical models to investigate the data, firstly we used RADEX models to fit the peak of the 12^{12}CO ladder, which in conjunction with the properties derived yielded a temperature of around 300 K. Subsequent numerical modeling with a full PDR model revealed that the dense phase has a filling factor of around 0.6 in both objects. The shape of the 12^{12}CO ladder was consistent with these components with heating dominated by grain photoelectric heating. An extra excitation component for the highest J lines (J > 20) is required for S 106.Comment: 20 pages, 10 figures, A&A Accepte

    Towards a Robuster Interpretive Parsing

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    The input data to grammar learning algorithms often consist of overt forms that do not contain full structural descriptions. This lack of information may contribute to the failure of learning. Past work on Optimality Theory introduced Robust Interpretive Parsing (RIP) as a partial solution to this problem. We generalize RIP and suggest replacing the winner candidate with a weighted mean violation of the potential winner candidates. A Boltzmann distribution is introduced on the winner set, and the distribution’s parameter TT is gradually decreased. Finally, we show that GRIP, the Generalized Robust Interpretive Parsing Algorithm significantly improves the learning success rate in a model with standard constraints for metrical stress assignment

    The characteristics of the IR emission features in the spectra of Herbig Ae stars: Evidence for chemical evolution

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    Herbig Ae/Be stars are a class of young pre-main sequence stellar objects of intermediate mass and are known to have varying amounts of natal cloud material still present in their direct vicinity. We characterise the IR emission bands, due to fluorescence by PAH molecules, in the spectra of Herbig Ae/Be stars and link observed variations to spatial aspects of the mid-IR emission. We analysed two PAH dominated spectra from a sample of 15 Herbig Ae/Be stars observed with Spitzer and derive profiles of the major PAH bands. The shape and the measured band characteristics show pronounced variations between the two Spitzer spectra. Those variations parallel those found between three ISO spectra of other, well-studied, Herbig Ae/Be stars. The derived profiles are compared to those from a broad sample of sources. The Spitzer and ISO spectra exhibit characteristics commonly interpreted respectively as interstellar matter-like (ISM), non-ISM-like, or a combination of the two. We argue that the PAH emission detected from the sources exhibiting a combination of ISM-like and non-ISM-like characteristics indicates the presence of two dissimilar, spatially separated, PAH families. As the shape of the individual PAH band profiles reflects the composition of the PAH molecules involved, this demonstrates that PAHs in subsequent, evolutionary linked stages of star formation are different from those in the general ISM, implying active chemistry. None of the detected PAH emission can be associated with the (unresolved) disk and is thus associated with the circumstellar cloud. This implies that chemical changes may already occur in the natal cloud and not necessarily in the disk

    Catch-up growth after prolonged hypothyroidism

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    Effects of high CO2 and warming on a Baltic Sea microzooplankton community

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    Global warming and ocean acidification are among the most important stressors for aquatic ecosystems in the future. To investigate their direct and indirect effects on a near-natural plankton community, a multiple-stressor approach is needed. Hence, we set up mesocosms in a full-factorial design to study the effects of both warming and high CO2 on a Baltic Sea autumn plankton community, concentrating on the impacts on microzooplankton (MZP). MZP abundance, biomass, and species composition were analysed over the course of the experiment. We observed that warming led to a reduced time-lag between the phytoplankton bloom and an MZP biomass maximum. MZP showed a significantly higher growth rate and an earlier biomass peak in the warm treatments while the biomass maximum was not affected. Increased pCO2 did not result in any significant effects on MZP biomass, growth rate, or species composition irrespective of the temperature, nor did we observe any significant interactions between CO2 and temperature. We attribute this to the high tolerance of this estuarine plankton community to fluctuations in pCO2, often resulting in CO2 concentrations higher than the predicted end-of-century concentration for open oceans. In contrast, warming can be expected to directly affect MZP and strengthen its coupling with phytoplankton by enhancing its grazing pressure

    Inzicht en toezicht: controle in de kennissamenleving

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    Nieuwe technieken maken het opslaan en verwerken van informatie eenvoudiger. Sterker\ud nog: ze maken de weg vrij om gegevens vast te leggen voordat duidelijk is welk inzicht\ud we eigenlijk nastreven. Toezicht wint zo terrein ten opzichte van de kennisverwerving.\ud \ud Voorbeelden van toenemend toezicht zijn elektronische dossiers over burgers,\ud informatievergaring door de politie en in private initiatieven zoals Google Earth. Deze\ud systemen maken het mogelijk om op grote schaal verbanden te ontdekken en afwijkingen op\ud te sporen, zonder dat er duidelijke kennisvragen aan vooraf gaan.\ud \ud De relatie tussen inzicht en toezicht is bepalend voor hoe we met de verzamelde kennis\ud omgaan. Ligt de nadruk daarbij op inzicht, overzicht, toezicht, of nog iets anders? Dit\ud Jaarboek Kennissamenleving 2010 stelt kritische vragen bij de alomtegenwoordige blik van\ud toezicht. Het draagt ideeën aan om deze in de toekomst anders te richten, zodat inzicht en\ud toezicht in balans kunnen blijven

    Double Neutron Star Systems and Natal Neutron Star Kicks

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    We study the four double neutron star systems found in the Galactic disk in terms of the orbital characteristics of their immediate progenitors and the natal kicks imparted to neutron stars. Analysis of the effect of the second supernova explosion on the orbital dynamics, combined with recent results from simulations of rapid accretion onto neutron stars lead us to conclude that the observed systems could not have been formed had the explosion been symmetric. Their formation becomes possible if kicks are imparted to the radio-pulsar companions at birth. We identify the constraints imposed on the immediate progenitors of the observed double neutron stars and calculate the ranges within which their binary characteristics (orbital separations and masses of the exploding stars) are restricted. We also study the dependence of these limits on the magnitude of the kick velocity and the time elapsed since the second explosion. For each of the double neutron stars, we derive a minimum kick magnitude required for their formation, and for the two systems in close orbits we find it to exceed 200km/s. Lower limits are also set to the center-of-mass velocities of double neutron stars, and we find them to be consistent with the current proper motion observations.Comment: 25 pages, 6 figs (9 parts), 4 tables, AASTeX, Accepted in Ap

    Cost-effectiveness analysis on elderly pneumococcal vaccination in the Netherlands:Challenging the Dutch Health Council's advice

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    Recently, the Dutch Health Council advised on elderly pneumococcal vaccination favouring the conventional polysaccharide vaccine over the novel conjugated vaccine. This advice was strongly inspired by a cost-effectiveness analysis considered to show favourable outcomes for the polysaccharide but not for the conjugated vaccine. We argue that using the same data and methods as presented by the Health Council, a different perspective on the results leads to a conclusion that not only the polysaccharide but also the conjugated pneumococcal vaccine is cost-effective. Our alternative perspective concerns the use of realistic vaccine prices, and applying an adequate time horizon for cost-effectiveness modelling. Notably, for one-off vaccination of 65-years old elderly, in all investigated analyses, also the conjugated vaccine seems cost-effective; i.e. well below the threshold of €20,000 per quality-adjusted life year, reflecting the most stringent threshold used for vaccines in the Netherlands
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