On the (non-)enhancement of the Lyman \alpha\ equivalent width by a multiphase interstellar medium

It has been suggested that radiative transfer effects may explain the unusually high equivalent widths (EWs) of the Lya line, observed occasionally from starburst galaxies, especially at high redshifts. If the dust is locked up inside high-density clouds dispersed in an empty intercloud medium, the Lya photons could scatter off of the surfaces of the clouds, effectively having their journey confined to the dustless medium. The continuum radiation, on the other hand, does not scatter, and would thus be subject to absorption inside the clouds. This scenario is routinely invoked when Lya EWs higher than what is expected theoretically are observed, although the ideal conditions under which the results are derived usually are not considered. Here we systematically examine the relevant physical parameters in this idealized framework, testing whether any astrophysically realistic scenarios may lead to such an effect. It is found that although clumpiness indeed facilitates the escape of Lya, it is highly unlikely that any real interstellar media should result in a preferential escape of Lya over continuum radiation. Other possible causes are discussed, and it is concluded that the observed high EWs are more likely to be caused by cooling radiation from cold accretion and/or anisotropic escape of the Lya radiation.Comment: Submitted to ApJ. Comments welcom

Galaxy formation from a timescale perspective

Timescales in astronomy comprise the largest range of any scientific discipline. In the construction of physical models, this circumstance may both be a blessing and a curse. For example, galaxy evolution occurs on typical timescales of hundreds of millions of years, but is affected by atomic processes on sub-second timescales, posing a challenge in analytical and, in particular, in numerical models. On the other hand, the vast dynamic range implies that we can often make meaningful predictions by simply comparing characteristic timescales of the physical processes involved. This review, aimed primarily at non-astronomer scientists, attempts to highlight some occasions in the context of galaxy formation and evolution in which comparing timescales can shed light on astrophysical phenomena, as well as some of the challenges that may be encountered. In particular we will explore the differences and similarities between theoretical predictions of dark matter halos, and the observed distribution of galaxies. The review concludes with an account of the most recent observations with the James Webb Space Telescope, and how they purportedly seem to defy the timescales of the currently accepted concordance model of the structure and evolution of the Universe, the {\Lambda}CDM model.Comment: A review-like tale of the physics leading to the formation of galaxies, aimed at non-astronomer scientists, but also of interest to students of astronomy, with several illustrative figures. Published on Springer Mathematics Online First Collections. To appear in the multidisciplinary anthology "Multiplicity of Time Scales in Complex Systems" (ed.: Dr. Bernhelm Booss-Bavnbek, Roskilde University

Macroeconomic Issues in Foreign Aid

The macroeconomic rationale for aid relates to its ability to supplem­ent savings, foreign exchange and government revenue, thus contributing to ­growth. This processes presumes a simple ­Harrod-Domar context in which growth is driven by physical capital formation. ­However, the macroeconomic reality of aid is more complicated. Three areas of complication are discussed: (i) the effects of aid on fiscal behaviour, (ii) debt problems and (iii) Dutch disease effects. In the long run, rather than merely filling gaps, aid should help close­ gaps, since reliance on future aid and foreign borrowing is thus diminished and economic policy autonomy is increased. Closing the savings gap entails financial and technical support for mobilisation of domestic savings. Closing the trade gap entails supporting a macro environment conducive to export growth, helping to expand and improve physical infrastructure and direct support for export activities, notably those of a non-traditional nature. Closing the fiscal gap entails support for increasing government revenue and improving expenditure management, which is the more delicate task since donors and recipient governments have to carefully balance the disadvantage of lower-than-needed government spending against the disadvantage of higher, and potentially distortionary, taxation.Foreign Aid; Macroeconomics of Aid; Gap Models; Aid Fungibility; Fiscal Response Models; Foreign Debt; Dutch Disease

Lyman-alpha line and continuum radiative transfer in a clumpy interstellar medium

Aims: We aim to study the effects of an inhomogeneous interstellar medium (ISM) on the strength and the shape of the Lyman alpha (Lya) line in starburst galaxies. Methods: Using our 3D Monte Carlo Lya radiation transfer code, we study the radiative transfer of Lya, UV and optical continuum photons in homogeneous and clumpy shells of neutral hydrogen and dust surrounding a central source. Our simulations predict the Lya and continuum escape fraction, the Lya equivalent width EW(Lya), the Lya line profile and their dependence on the gas geometry and the main input physical parameters. Results: The ISM clumpiness is found to have a strong impact on the Lya line radiative transfer, entailing a strong dependence of the emergent features of the Lya line (escape fraction, EW(Lya)) on the ISM morphology. Although a clumpy and dusty ISM appears more transparent to radiation (both line and continuum) compared to an equivalent homogeneous ISM of equal dust optical depth, we find that the Lya photons are, in general, still more attenuated than UV continuum radiation. As a consequence, the observed Lya equivalent width (EWobs(Lya)) is lower than the intrinsic one (EWint(Lya)) for nearly all clumpy ISM configurations considered. There are, however, special conditions under which Lya photons escape more easily than the continuum, resulting in an enhanced EWobs(Lya). The requirement for this to happen is that the ISM is almost static (galactic outflows < 200 km/s), extremely clumpy (with density contrasts >10^7 in HI between clumps and the interclump medium), and very dusty (E(B-V) > 0.30). When these conditions are fulfilled the emergent Lya line profile shows no velocity shift and little asymmetry. Given the asymmetry and velocity shifts generally observed in starburst galaxies with Lya emission, we conclude that clumping is unlikely to significantly enhance their relative Lya/UV transmission.Comment: 20 pages, 22 figures. Accepted for publication in A&

Intergalactic Transmission and its Impact on the Ly{\alpha} Line

We study the intergalactic transmission of radiation in the vicinity of the Ly{\alpha} wavelength. Simulating sightlines through the intergalactic medium (IGM) in detailed cosmological hydrosimulations, the impact of the IGM on the shape of the line profile from Ly{\alpha} emitting galaxies at redshifts 2.5 to 6.5 is investigated. In particular we show that taking into account the correlation of the density and velocity fields of the IGM with the galaxies, the blue part of the spectrum may be appreciably reduced, even at relatively low redshifts. This may in some cases provide an alternative to the often-invoked outflow scenario, although it is concluded that this model is still a plausible explanation of the many asymmetric Ly{\alpha} profiles observed. Applying the calculated wavelength dependent transmission to simulated spectra from Ly{\alpha} emitting galaxies, we derive the fraction of photons that are lost in the IGM, in addition to what is absorbed internally in the galaxies due to dust. Moreover, by comparing the calculated transmission of radiation blueward of the Ly{\alpha} line, the total optical depth to Thomson scattering of cosmic microwave background, with corresponding observations, we are able to constrain the epoch when the Universe was reionized to z <~ 8.5.Comment: Substantially extended, ~30 references added, 1.5 page extra (article style) in particular on the impact of the IGM at z~5.8 and z~6.5, 2 extra figures, unnecessary fluff cut out, accepted for publication in Ap

Lyman alpha Resonant Scattering in Young Galaxies - Predictions from Cosmological Simulations

We present results obtained with a 3D, Ly alpha radiative transfer code, applied to a fully cosmological galaxy formation simulation. The developed Monte Carlo code is capable of treating an arbitrary distribution of source Ly alpha emission, neutral hydrogen density, temperature, and peculiar velocity of the interstellar medium. We investigate the influence of resonant scattering on the appearance and properties of young galaxies by applying the code to a simulated "Lyman Break Galaxy" at redshift z = 3.6, and of star formation rate 22 M_sun/yr and total Ly alpha luminosity 2.0 X 10^43 erg/s. It is found that resonant scattering of Ly alpha radiation can explain that young galaxies frequently are observed to be more extended on the sky in Ly alpha than in the optical. Moreover, it is shown that, for the system investigated, due to the anisotropic escape of the photons, the appearent maximum surface brightness can differ by a factor of ~15, and the total derived luminosity by a factor of ~4, depending on the orientation of the system relative to the observer.Comment: Letter updated to match version published in Ap

SE-ENRICHMENT OF CARROT AND ONION VIA FOLIAR APPLICATION

The aim of this work was to study the selenium accumulation in carrot and onion plants using foliar application by sodium selenite and sodium selenate. Furthermore, we aimed at identifying the Se species biosynthesised by onion and carrot plants. The results were used to prepare for production of 77Se enriched plants for an ongoing human absorption study

Finite-Element Limit Analysis of the Tucker High School Gymnasium Roof Failure

The Randolph Tucker High School gymnasium roof failure of 1970 has received much scholarly attention. This study will provide a conclusion to a large body of previously published works by means of limit state analysis of the roof failure using state of the art parametric finite-element modeling. Parametric modeling within a general purpose finite-element analysis program allows for extremely rapid changes to the model because key terms are objects or parameters that can be adjusted internally by the program, rather than laboriously entered by the user. The failure of the roof was investigated by means of a limit state analysis, which accurately captured the cracking of the concrete and the yielding of the reinforcing steel. Concrete creep and shrinkage and relaxation of the prestressing steel were also accounted for. Finally, the authors also studied the idea that camber in the roof geometry might have prevented collapse