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„Wir schaffen das!“
(2016)
„Vajanie iz vremeni“
(2016)
Die Worte „entjuden“ und „Entjudung“ sind sprachlicher Ausdruck zumeist judenfeindlicher Haltungen und Taten in der deutschen Geschichte. Der Beitrag zeichnet die Entwicklung des Begriffs anhand seiner Verwendungszusammenhänge nach. Im Kontext der Assimilation des beginnenden 19. Jahrhunderts meinte der Terminus, dass man sich jener jüdischen „Eigenheit“ zu entkleiden habe, welche als Postulat gemeinhin Konsens war. Innerhalb der innerjüdischen Diskussion wird „Entjudung“ zu Beginn des 20. Jahrhunderts zum diagnostischen Ausdruck des Identitätsverlustes. Als politischer Kampfbegriff der Nationalsozialisten ist er wiederum zum Synonym für die Entrechtung und Vernichtung jüdischer Menschen geworden. Protestantische Theologen verwendeten diesen Begriff in der Debatte um die Erneuerung des Christentums, was durch die Entfernung jüdischer Einflüsse geschehen sollte. Bereits Ende des 18. Jahrhunderts formuliert, findet diese Forderung in der 1939 erfolgten Gründung des Instituts zur Erforschung und Beseitigung des jüdischen Einflusses auf das deutsche kirchliche Leben seine programmatische Umsetzung.
Тезисы
(2016)
Тезисы
(2016)
Тезисы
(2016)
Тезисы
(2016)
Тезисы
(2016)
Тезисы
(2016)
Солярис как процесс
(2016)
О новых истоках кино
(2016)
In an eye-tracking study we tested the hypothesis that comprehension is facilitated by a match between the order of the verb and its arguments in a sentence and the order of the actual sensorimotor interaction with these objects (for example, in the phrase put the bag into the box, the order of the arguments corresponds to the order of motor actions: take the bag, put it into the box) could facilitate comprehension of such constructions. We tested 40 native Russian speakers in a visual world sentence-picture matching task. In prepositional constructions, there was no difference between conditions that matched or mismatched sensorimotor stereotypes, whereas in instrumental constructions, sensorimotor stereotypes facilitated comprehension.
Блуждающие цитаты
(2016)
Биографические мотивы условно можно разделить на два вида:
1. Отдельные небольшие эпизоды или впечатления, запомнившие-
ся Тарковскому, которые заняли свое точное место в его сценариях и
фильмах. Режиссер А. Гордон условно назвал этот прием Тарковского
«теорией пазлов». Такие элементы встречаются почти во всех фильмах
Андрея Тарковского.
2. Расширенное включение в фильмы автобиографии, естественно, не
во всей полноте. К таким фильмам относятся Зеркало (1974) и Offret
(«Жертвоприношение» – 1986).
After the mass immigration to Israel from 1948 to 1950, about 2000 Jews remained
in Yemen. These Jews lived in small communities and continued to maintain their
religious environment as it was. In the years that followed, many of them, however, moved from Yemen to Israel with the assistance of the Jewish Agency and the Joint
Distribution Committee (JDC). The community was of a small size and the fact that it
was dispersed throughout the predominantly Muslim areas, created a certain closeness
between the two groups. About ten percent of the Jews chose to convert to Islam, many
of them in groups. In about twenty cases, the husbands chose to convert to Islam while
their wives emigrated to preserve their Judaism. Some of the converts refused to grant
their wives a divorce, because, according to Muslim law, conversion is enough to sever
the marital relationship. This procedure is called ʿAgunot. Meaning, women bound in
marriage to a husband and they no longer lived together, but the husband didn’t formally
‘released’ her from marriage union. The article follows the efforts undertaken
to release the ʿAgunot, and shows that Jewish and Muslim scholars were able to find
solutions to the ʿAgunot problem and, at times, managed to bridge the gap between the
two religions.
Černobylʼ, Gewalt, Mythos
(2016)
Im vorliegenden Beitrag werden einige zentrale Berichte und Motive aus den frühen Quellen des Islam über die militärischen Konflikte des Propheten Muhammad mit den
Juden von Medina beleuchtet. Als Grundlage der Untersuchung dient die Prophetenbiografie des Gelehrten Muḥammad ibn Isḥāq (gest. 150 nach der Hedschra), die auch heute noch maßgeblich ist. Im Beitrag wird unter anderem aufgezeigt, dass es sowohl innerhalb der Gattung der Sīra-Literatur, der Ibn Isḥāqs Werk angehört, als auch in den frühen Traditionen der islamischen Rechtswissenschaft, der Koranexegese sowie im Korantext selbst zahlreiche Hinweise auf alternative Darstellungen dieser Konflikte gibt. Diese gerieten in den ersten Jahrhunderten des Islam infolge des Siegeszuges von Ibn Isḥāqs Werk zunehmend aus dem Blickfeld, sind aber für zeitgenössische Diskurse um das Verhältnis des Islam zu Nichtmuslimen durchaus von Interesse. Ziel der Untersuchung ist es die normative Aussagekraft der unterschiedlichen Szenarien für Grundsatzfragen insbesondere für das Verhältnis zwischen Muslimen und Juden herauszuarbeiten. Einen inhaltlichen Schwerpunkt im Beitrag bilden dabei unterschiedliche Zugänge zum berühmten Bericht über die Vernichtung des jüdischen Stammes der Banū Qurayza im Anschluss an die Grabenschlacht.
La référence à Colomb est un lieu commun de la biographie humboldtienne. Humboldt lui-même le souligne particulièrement dans son Examen critique, en y ajoutant une dimension autobiographique. La contribution analyse, dans une perspective philologique, le matériel et les formes de mise en scène avec lesquelles une vie est représentée au travers d'une autre.
Zurück am Neuen Palais
(2016)
Zum Hundertsten nichts Neues
(2016)
Yolk@Shell Nanoarchitectures with Bimetallic Nanocores - Synthesis and Electrocatalytic Applications
(2016)
The spatial magnetic properties (Through Space NMR Shieldings - TSNMRS) of a number of Y-shaped structures possessing 4n+2 pi-electrons (i.a. the trimethylenemethane ions TMM2+, TMM2-, the guanidinium cation, substituted and hetero analogues) have been computed, visualized as Isochemical Shielding Surfaces (ICSS) of various size and direction, were examined subject to present Y-aromaticity and the results compared with energetic and geometric criteria obtained already. (C) 2016 Elsevier Ltd. All rights reserved.
XVII. Proper motions of the Small Magellanic Cloud and the Milky Way globular cluster 47 Tucanae
(2016)
Aims. In this study we use multi-epoch near-infrared observations from the VISTA survey of the Magellanic Cloud system (VMC) to measure the proper motions of different stellar populations in a tile of 1.5 deg2 in size in the direction of the Galactic globular cluster 47 Tuc. We obtain the proper motion of the cluster itself, of the Small Magellanic Cloud (SMC), and of the field Milky Way stars.
Methods. Stars of the three main stellar components are selected according to their spatial distributions and their distributions in colour−magnitude diagrams. Their average coordinate displacement is computed from the difference between multiple Ks-band observations for stars as faint as Ks = 19 mag. Proper motions are derived from the slope of the best-fitting line among ten VMC epochs over a time baseline of ~1 yr. Background galaxies are used to calibrate the absolute astrometric reference frame.
Results. The resulting absolute proper motion of 47 Tuc is (μαcos(δ), μδ) = (+7.26 ± 0.03, −1.25 ± 0.03) mas yr-1. This measurement refers to about 35 000 sources distributed between 10′ and 60′ from the cluster centre. For the SMC we obtain (μαcos(δ), μδ) = (+1.16 ± 0.07, −0.81 ± 0.07) mas yr-1 from about 5250 red clump and red giant branch stars. The absolute proper motion of the Milky Way population in the line of sight (l = 305.9, b = −44.9) of this VISTA tile is (μαcos(δ), μδ) = (+10.22 ± 0.14, −1.27 ± 0.12) mas yr-1 and has been calculated from about 4000 sources. Systematic uncertainties associated with the astrometric reference system are 0.18 mas yr-1. Thanks to the proper motion we detect 47 Tuc stars beyond its tidal radius.
X-RAY OBSERVATIONS OF BOW SHOCKS AROUND RUNAWAY O STARS. THE CASE OF zeta OPH AND BD+43 degrees 3654
(2016)
Non-thermal radiation has been predicted within bow shocks around runaway stars by recent theoretical works. We present X-ray observations toward the runaway stars zeta Oph by Chandra and Suzaku and of BD+43 degrees 3654 by XMM-Newton to search for the presence of non-thermal X-ray emission. We found no evidence of non-thermal emission spatially coincident with the bow shocks; nonetheless, diffuse emission was detected in the vicinity of zeta Oph. After a careful analysis of its spectral characteristics, we conclude that this emission has a thermal nature with a plasma temperature of T approximate to 2 x 10(6) K. The cometary shape of this emission seems to be in line with recent predictions of radiation-hydrodynamic models of runaway stars. The case of BD+43 degrees 3654 is puzzling, as non-thermal emission has been reported in a previous work for this source.
Nearly all types of massive stars with radiatively driven stellar winds are X-ray sources that can be observed by the presently operating powerful X-ray telescopes. In this review I briefly address recent advances in our understanding of stellar winds obtained from X-ray observations. X-rays may strongly influence the dynamics of weak winds of main sequence B-type stars. X-ray pulsations were detected in a beta Cep type variable giving evidence of tight photosphere-wind connections. The winds of OB dwarfs with subtypes later than O9V may be predominantly in a hot phase, and X-ray observations offer the best window for their studies. The X-ray properties of OB super giants are largely determined by the effects of radiative transfer in their clumped stellar winds. The recently suggested method to directly measure mass-loss rates of O stars by fitting the shapes of X-ray emission lines is considered but its validity cannot be confirmed. To obtain robust quantitative information on stellar wind parameters from X-ray spectroscopy, a multiwavelength analysis by means of stellar atmosphere models is required. Independent groups are now performing such analyses with encouraging results. Joint analyses of optical, UV, and X-ray spectra of OB supergiants yield consistent mass-loss rates. Depending on the adopted clumping parameters, the empirically derived mass-loss rates are a factor of a few smaller or comparable to those predicted by standard recipes (Vink et al., 2001). All sufficiently studied O stars display variable X-ray emission that might be related to corotating interaction regions in their winds. In the latest stages of stellar evolution, single red supergiants (RSG) and luminous blue variable (LBV) stars do not emit observable amounts of X-rays. On the other hand, nearly all types of Wolf-Rayet (WR) stars are X-ray sources. X-ray spectroscopy allows a sensitive probe of WR wind abundances and opacities. (C) 2016 COSPAR. Published by Elsevier Ltd. All rights reserved.
X-ray free electron lasers (XFELs) enable unprecedented new ways to study the electronic structure and dynamics of transition metal systems. L-edge absorption spectroscopy is a powerful technique for such studies and the feasibility of this method at XFELs for solutions and solids has been demonstrated. However, the required x-ray bandwidth is an order of magnitude narrower than that of self-amplified spontaneous emission (SASE), and additional monochromatization is needed. Here we compare L-edge x-ray absorption spectroscopy (XAS) of a prototypical transition metal system based on monochromatizing the SASE radiation of the linac coherent light source (LCLS) with a new technique based on self-seeding of LCLS. We demonstrate how L-edge XAS can be performed using the self-seeding scheme without the need of an additional beam line monochromator. We show how the spectral shape and pulse energy depend on the undulator setup and how this affects the x-ray spectroscopy measurements. (C) 2016 Optical Society of America
Language and communication disorders are often associated with deficits in working memory (WM) and interference control. WM studies involving children with specific language impairment (SLI) have traditionally been framed using either resource theories or decay accounts, particularly Baddeley's model. Although significant interference problems in children with SLI are apparent in error analysis data from WM and language tasks, interference theories and paradigms have not been widely used in the SLI literature. A primary goal of the present paper is to provide an overview of interference deficits in children with SLI. Review of the extant literature on interference control shows deficits in this population; however, the source and the nature of the deficit remain unclear. Thus, a second key aim in our review is to demonstrate the need for theoretically driven experimental paradigms in order to better understand individual variations associated with interference weaknesses in children with SLI.
Objective: The aim of this study was to study the effects of a short-term cognitive behavior therapy on work-anxiety and sickness-absence in patients with work-anxiety. Methods: Three-hundred forty-five inpatients who suffered from cardiologic, neurological, or orthopedic problems and additionally work-anxiety were randomly assigned into two different group interventions. Patients got four sessions of a group intervention, which either focused on cognitive behavior-therapy anxiety-management (work-anxiety coping group, WAG) or unspecific recreational activities (RG). Results: No differences were found between WAG and RG for work-anxiety and subjective work ability. When looking at patients who were suffering only from work-anxiety, and no additional mental disorder, the duration of sickness absence until 6 months follow-up was shorter in the WAG (WAG: 11 weeks, RG: 16 weeks, P = 0.050). Conclusion: A shortterm WAG may help return to work in patients with work-anxieties, as long as there is no comorbid mental disorder.