@article{CoetzeeVanRooyPeters2021, author = {Coetzee-Van Rooy, Susan and Peters, Arne}, title = {A portrait-corpus study of language attitudes towards Afrikaans and English}, series = {Language matters : studies in the languages of Africa}, volume = {52}, journal = {Language matters : studies in the languages of Africa}, number = {2}, publisher = {Routledge, Taylor \& Francis Group}, address = {Abingdon}, issn = {1022-8195}, doi = {10.1080/10228195.2021.1942167}, pages = {3 -- 28}, year = {2021}, abstract = {Language portraits are useful instruments to elicit speakers' reflections on the languages in their repertoires. In this study, we implement a "portrait-corpus approach" (Peters and Coetzee-Van Rooy 2020) to investigate the conceptualisations of the languages Afrikaans and English in 105 language portraits. In this approach, we use participants' reflections about their placement of the two languages on a human silhouette as a linguistic corpus. Relying on quantitative and qualitative analyses using WordSmith, Statistica and Atlas.ti, our study shows that Afrikaans is mainly conceptualised as a language that is located in more peripheral areas of the body (for example, the hands and feet) and, hence, is perceived as less important in participants' repertoires. The central location of English in the head reveals its status as an important language in the participants' multilingual repertoires. We argue that these conceptualisations of Afrikaans and English provide additional insight into the attitudes towards these languages in South Africa.}, language = {en} } @article{RichterCharltonFanganoetal.2009, author = {Richter, Philipp and Charlton, Jane C. and Fangano, Alessio P. M. and Ben Bekhti, Nadya and Masiero, Joseph R.}, title = {A population of weak metal-line absorbers surrounding the Milky Way}, issn = {0004-637X}, doi = {10.1088/0004-637x/695/2/1631}, year = {2009}, abstract = {We report on the detection of a population of weak metal-line absorbers in the halo or nearby intergalactic environment of the Milky Way. Using high-resolution ultraviolet absorption-line spectra of bright quasars (QSO) obtained with the Space Telescope Imaging Spectrograph (STIS), along six sight lines we have observed unsaturated, narrow absorption in O I and Si II, together with mildly saturated C II absorption at high radial velocities (vertical bar v(LSR)vertical bar = 100-320 km s(-1)). The measured O I column densities lie in the range N(O I) 2 x 10(14) cm(-2) implying that these structures represent Lyman limit Systems and sub-Lyman limit System with H I column densities between 10(16) and 3 x 10(18) cm(-2), thus below the detection limits of current 21 cm all-sky surveys of high-velocity clouds (HVCs). The absorbers apparently are not directly associated with any of the large high column density HVC complexes, but rather represent isolated, partly neutral gas clumps embedded in a more tenuous, ionized gaseous medium situated in the halo or nearby intergalactic environment of the Galaxy. Photoionization modeling of the observed low ion ratios suggests typical hydrogen volume densities of n(H) > 0.02 cm(-3) and characteristic thicknesses of a several parsec down to subparsec scales. For three absorbers, metallicities are constrained in the range of 0.1-1.0 solar, implying that these gaseous structures may have multiple origins inside and outside the Milky Way. Using supplementary optical absorption-line data, we find for two other absorbers Ca II/O I column-density ratios that correspond to solar Ca/O abundance ratios. This finding indicates that these clouds do not contain significant amounts of dust. This population of low column density gas clumps in the circumgalactic environment of the Milky Way is indicative of the various processes that contribute to the circulation of neutral gas in the extended halos of spiral galaxies. These processes include the accretion of gas from the intergalactic medium and satellite galaxies, galactic fountains, and outflows. We speculate that this absorber population represents the local analog of weak Mg II systems that are commonly observed in the circumgalactic environment of low- and high-redshift galaxies.}, language = {en} } @article{BoumaRichterFechner2019, author = {Bouma, Sietske Jeltje Deirdre and Richter, Philipp and Fechner, Cora}, title = {A population of high-velocity absorption-line systems residing in the Local Group}, series = {Astronomy and astrophysics : an international weekly journal}, volume = {627}, journal = {Astronomy and astrophysics : an international weekly journal}, publisher = {EDP Sciences}, address = {Les Ulis}, issn = {1432-0746}, doi = {10.1051/0004-6361/201935078}, pages = {12}, year = {2019}, abstract = {Aims. We investigated the ionisation conditions and distances of Galactic high-velocity clouds (HVCs) in the Galactic halo and beyond in the direction of the Local Group (LG) barycentre and anti-barycentre, by studying spectral data of 29 extragalactic background sources obtained with the Cosmic Origins Spectropgraph (COS) installed on the Hubble Space Telescope (HST). Methods. We model column-densities of low, intermediate, and high ions such as Si ii, C ii, Si iii, Si vi, and C iv, and use these data to construct a set of Cloudy ionisation models. Results. In total, we found 69 high-velocity absorption components along the 29 lines of sight. The components in the direction of the LG barycentre span the entire range of studied velocities, 100 less than or similar to vertical bar nu(LSR)vertical bar less than or similar to 400 km s(-1), while those in the anti-barycentre sample have velocities up to about 300 km s(-1). For 49 components, we infer the gas densities. In the direction of the LG barycentre, the gas densities exhibit a wide range from log nH = -3.96 to -2.55, while in the anti-barycentre direction the densities are systematically higher, log nH > -3.25. The barycentre absorbers can be split into two groups based on their density: a high-density group with log nH > -3.54, which can be affected by the Milky Way radiation field, and a low-density group (log nH <= -3.54). The latter has very low thermal pressures of P/k < 7.3 Kcm(-3). Conclusions. Our study shows that part of the absorbers in the LG barycentre direction trace gas at very low gas densities and thermal pressures. These properties indicate that the absorbers are located beyond the virial radius of the Milky Way. Our study also confirms results from earlier, single-sightline studies, suggesting the presence of a metal-enriched intragroup medium filling the LG near its barycentre.}, language = {en} } @article{PearceSarsakovSchaubetal.2002, author = {Pearce, David and Sarsakov, Vladimir and Schaub, Torsten and Tompits, Hans and Woltran, Stefan}, title = {A polynomial translation of logic programs with nested expressions into disjunctive logic programs : preliminary report}, year = {2002}, language = {en} } @article{PearceSarsakovSchaubetal.2002, author = {Pearce, David and Sarsakov, Vladimir and Schaub, Torsten and Tompits, Hans and Woltran, Stefan}, title = {A polynomial translation of logic programs with nested expressions into disjunctive logic programs}, isbn = {3-540-43930-7}, year = {2002}, language = {en} } @article{ThielZehbeRoesneretal.2013, author = {Thiel, Kerstin and Zehbe, Rolf and Roesner, Jer{\^o}m{\´e} and Strauch, Peter and Enthaler, Stephan and Thomas, Arne}, title = {A polymer analogous reaction for the formation of imidazolium and NHC based porous polymer networks}, doi = {10.1039/C2PY20947K}, year = {2013}, abstract = {A polymer analogous reaction was carried out to generate a porous polymeric network with N-heterocyclic carbenes (NHC) in the polymer backbone. Using a stepwise approach, first a polyimine network is formed by polymerization of the tetrafunctional amine tetrakis(4-aminophenyl)methane. This polyimine network is converted in the second step into polyimidazolium chloride and finally to a polyNHC network. Furthermore a porous Cu(II)-coordinated polyNHC network can be generated. Supercritical drying generates polymer networks with high permanent surface areas and porosities which can be applied for different catalytic reactions. The catalytic properties were demonstrated for example in the activation of CO2 or in the deoxygenation of sulfoxides to the corresponding sulfides.}, language = {en} } @article{ThielZehbeRoeseretal.2013, author = {Thiel, Kerstin and Zehbe, Rolf and R{\"o}ser, Jerome and Strauch, Peter and Enthaler, Stephan and Thomas, Arne}, title = {A polymer analogous reaction for the formation of imidazolium and NHC based porous polymer networks}, series = {Polymer Chemistry}, volume = {4}, journal = {Polymer Chemistry}, number = {6}, publisher = {Royal Society of Chemistry}, address = {Cambridge}, issn = {1759-9954}, doi = {10.1039/c2py20947k}, pages = {1848 -- 1856}, year = {2013}, abstract = {A polymer analogous reaction was carried out to generate a porous polymeric network with N-heterocyclic carbenes (NHC) in the polymer backbone. Using a stepwise approach, first a polyimine network is formed by polymerization of the tetrafunctional amine tetrakis(4-aminophenyl)methane. This polyimine network is converted in the second step into polyimidazolium chloride and finally to a polyNHC network. Furthermore a porous Cu(II)-coordinated polyNHC network can be generated. Supercritical drying generates polymer networks with high permanent surface areas and porosities which can be applied for different catalytic reactions. The catalytic properties were demonstrated for example in the activation of CO2 or in the deoxygenation of sulfoxides to the corresponding sulfides.}, language = {en} } @article{LiaimerJenkeKodamaIshidaetal.2011, author = {Liaimer, Anton and Jenke-Kodama, Holger and Ishida, Keishi and Hinrichs, Katrin and Stangeland, Janne and Hertweck, Christian and Dittmann-Th{\"u}nemann, Elke}, title = {A polyketide interferes with cellular differentiation in the symbiotic cyanobacterium Nostoc punctiforme}, series = {Environmental microbiology reports}, volume = {3}, journal = {Environmental microbiology reports}, number = {5}, publisher = {Wiley-Blackwell}, address = {Malden}, issn = {1758-2229}, doi = {10.1111/j.1758-2229.2011.00258.x}, pages = {550 -- 558}, year = {2011}, abstract = {Nostoc punctiforme is a filamentous cyanobacterium capable of forming symbiotic associations with a wide range of plants. The strain exhibits extensive phenotypic characteristics and can differentiate three mutually exclusive cell types: nitrogen-fixing heterocysts, motile hormogonia and spore-like akinetes. Here, we provide evidence for a crucial role of an extracellular metabolite in balancing cellular differentiation. Insertional mutagenesis of a gene of the polyketide synthase gene cluster pks2 led to the accumulation of short filaments carrying mostly terminal heterocysts under diazotrophic conditions. The mutant has a strong tendency to form biofilms on solid surfaces as well as in liquid culture. The pks2-strain keeps forming hormogonia over the entire growth curve and shows an early onset of akinete formation. We could isolate two fractions of the wildtype supernatant that could restore the capability to form long filaments with intercalary heterocysts. Growth of the mutant cells in the neighbourhood of wild-type cells on plates led to a reciprocal influence and a partial reconstruction of wild-type and mutant phenotype respectively. We postulate that extracellular metabolites of Nostoc punctiforme act as life cycle governing factors (LCGFs) and that the ratio between distinct factors may guide the differentiation into different life stages.}, language = {en} } @article{KlemmHerzschuhPisaricetal.2013, author = {Klemm, Juliane and Herzschuh, Ulrike and Pisaric, Michael F. J. and Telford, Richard J. and Heim, Birgit and Pestryakova, Luidmila Agafyevna}, title = {A pollen-climate transfer function from the tundra and taiga vegetation in Arctic Siberia and its applicability to a Holocene record}, series = {Palaeogeography, palaeoclimatology, palaeoecology : an international journal for the geo-sciences}, volume = {386}, journal = {Palaeogeography, palaeoclimatology, palaeoecology : an international journal for the geo-sciences}, publisher = {Elsevier}, address = {Amsterdam}, issn = {0031-0182}, doi = {10.1016/j.palaeo.2013.06.033}, pages = {702 -- 713}, year = {2013}, abstract = {This study aims to establish, evaluate, and apply a modern pollen-climate transfer function from the transition zone between arctic tundra and light-needled taiga in Arctic Siberia. Lacustrine samples (n = 96) from the northern Siberian lowlands of Yakutia were collected along four north-to-south transects crossing the arctic forest line. Samples span a broad temperature and precipitation gradient (mean July temperature, T-July: 7.5-18.7 degrees C; mean annual precipitation, P-ann: 114-315 mm/yr). Redundancy analyses are used to examine the relationship between the modern pollen signal and corresponding vegetation types and climate. Performance of transfer functions for T-July and P-ann were cross-validated and tested for spatial autocorrelation effects. The root mean square errors of prediction are 1.67 degrees C for T-July and 40 mm/yr for P-ann. A climate reconstruction based on fossil pollen spectra from a Siberian Arctic lake sediment core spanning the Holocene yielded cold conditions for the Late Glacial (1-2 degrees C below present T-July). Warm and moist conditions were reconstructed for the early to mid Holocene (2 degrees C higher T-July than present), and climate conditions similar to modern ones were reconstructed for the last 4000 years. In conclusion, our modern pollen data set fills the gap of existing regional calibration sets with regard to the underrepresented Siberian tundra-taiga transition zone. The Holocene climate reconstruction indicates that the temperature deviation from modern values was only moderate despite the assumed Arctic sensitivity to present climate change.}, language = {en} } @article{Paessler2017, author = {P{\"a}ßler, Ulrich}, title = {A Political Economy of Nature}, series = {HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies}, volume = {XVIII}, journal = {HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies}, number = {34}, publisher = {Universit{\"a}tsverlag Potsdam}, address = {Potsdam}, issn = {1617-5239}, doi = {10.18443/252}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-395781}, pages = {80 -- 91}, year = {2017}, abstract = {In seinem Aufsatz „Ueber die Schwankungen der Goldproduktion mit R{\"u}cksicht auf staatswirthschaftliche Probleme" (1838) entfaltet Alexander von Humboldt auf wenigen Seiten eine Weltgeschichte des Edelmetallverkehrs von der Antike bis ins 19. Jahrhundert. Der vorliegende Artikel geht Humboldts {\"o}konomischem Denken als Teil seiner Forschungen zur Natur- und Menschheitsgeschichte nach. Er beginnt mit einem kurzen Abriss der von sp{\"a}tmerkantilistischen und fr{\"u}hliberalen Einfl{\"u}ssen gepr{\"a}gten Ausbildung Humboldts. Der Artikel diskutiert anschließend eine von Humboldt angefertigte Weltkarte sowie vier darauf bezogene Schaubilder, die historische und zeitgen{\"o}ssische statistische Daten zur graphischen Vision eines globalen Wirtschaftskreislaufs kombinieren. In einem weiteren Schritt geht der Artikel Humboldts Anwendung historischer und naturgeschichtlicher Forschungsmethoden auf dem Gebiet der politischen {\"O}konomie am Beispiel des Aufsatzes von 1838 nach. Den Schluss der Untersuchung bildet Humboldts Auseinandersetzung mit dem Edelmetall Platin, dessen begrenzte Verbreitung im Widerspruch zur Idee eines freien weltweiten Austauschs stand.}, language = {en} }