scholarly journals Voices of Płaszów: The Impact of Schindler's List on a Former Concentration Camp

2020 ◽  
Author(s):  
Jordan L Riggs
2015 ◽  
Vol 24 (2) ◽  
pp. 190-202
Author(s):  
Florian Alix-Nicolaï

Ernst Toller's Pastor Hall, one of the first plays to depict life in a concentration camp, counts among the few anti-Nazi dramas translated into English before World War Two. The process by which it came to the British stage reveals the impact of censorship on authors and translators of anti-Fascist plays. It also reveals conflicting aesthetic strategies to tackle fascism. While Toller relied on straightforward documentary realism, one of his translators, W. H. Auden, championed anti-illusionism and distrusted propaganda art. In the cultural fight to reclaim Germany's heritage from the Nazis, German writers in exile viewed translations as urgent messages demanding prompt action, whereas British writers tended to see them as an archive for future generations.


2019 ◽  
Vol 9 (3-4) ◽  
pp. 181-189
Author(s):  
Stefan Konstańczak

Abstract In the article, the author analyses the impact of the tragic experiences during the Holocaust on contemporary ethics and literature. Such considerations coincide with yet another anniversary – the liberation of the Auschwitz concentration camp, celebrated globally as Holocaust Memorial Day. The article also considers the reasons why testimonies from Holocaust survivors have not had an adequate impact on society. The author argues that trivialisation of the Holocaust tragedy occurred in modern science and it is related to the fact that traditional ethics has not been able to convincingly explain why the Holocaust occurred in the most civilised nations. Thus, Holocaust testimonies should be constantly popularised in society for the good of all mankind. Literature seems to be the best form of mass media for this task and it is also a recorder of human emotions. According to the author, it is essential that humanity is protected this way against the possibility of a similar tragedy occurring in the future.


2019 ◽  
Vol 6 (4) ◽  
pp. 205316801989137 ◽  
Author(s):  
Julian M. Hoerner ◽  
Alexander Jaax ◽  
Toni Rodon

Of all atrocities committed by state actors in 20th century Europe, the systematic killings by Nazi Germany were arguably the most severe and best documented. While several studies have investigated the impact of the presence of concentration camps on surrounding communities in Germany and the occupied territories in terms of redistribution of wealth and property, the local-level impact on voting behaviour has not yet been explored. We investigated the impact of spatial proximity to a concentration camp between 1933 and 1945 on the likelihood of voting for far-right parties in the 2013 and 2017 federal elections. We find that proximity to a former concentration camp is associated with a higher vote share of such parties. A potential explanation for this finding could be a ‘memory satiation effect’, according to which voters who live in close proximity to former camps and are more frequently confronted with the past are more receptive to revisionist historical accounts questioning the centrality of the Holocaust in the German culture of remembrance.


1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.


1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.


1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.


1997 ◽  
Vol 161 ◽  
pp. 179-187
Author(s):  
Clifford N. Matthews ◽  
Rose A. Pesce-Rodriguez ◽  
Shirley A. Liebman

AbstractHydrogen cyanide polymers – heterogeneous solids ranging in color from yellow to orange to brown to black – may be among the organic macromolecules most readily formed within the Solar System. The non-volatile black crust of comet Halley, for example, as well as the extensive orangebrown streaks in the atmosphere of Jupiter, might consist largely of such polymers synthesized from HCN formed by photolysis of methane and ammonia, the color observed depending on the concentration of HCN involved. Laboratory studies of these ubiquitous compounds point to the presence of polyamidine structures synthesized directly from hydrogen cyanide. These would be converted by water to polypeptides which can be further hydrolyzed to α-amino acids. Black polymers and multimers with conjugated ladder structures derived from HCN could also be formed and might well be the source of the many nitrogen heterocycles, adenine included, observed after pyrolysis. The dark brown color arising from the impacts of comet P/Shoemaker-Levy 9 on Jupiter might therefore be mainly caused by the presence of HCN polymers, whether originally present, deposited by the impactor or synthesized directly from HCN. Spectroscopic detection of these predicted macromolecules and their hydrolytic and pyrolytic by-products would strengthen significantly the hypothesis that cyanide polymerization is a preferred pathway for prebiotic and extraterrestrial chemistry.


Author(s):  
Lucien F. Trueb

Crushed and statically compressed Madagascar graphite that was explosively shocked at 425 kb by means of a planar flyer-plate is characterized by a black zone extending for 2 to 3 nun below the impact plane of the driver. Beyond this point, the material assumes the normal gray color of graphite. The thickness of the black zone is identical with the distance taken by the relaxation wave to overtake the compression wave.The main mechanical characteristic of the black material is its great hardness; steel scalpels and razor blades are readily blunted during attempts to cut it. An average microhardness value of 95-3 DPHN was obtained with a 10 kg load. This figure is a minimum because the indentations were usually cracked; 14.8 DPHN was measured in the gray zone.


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