Author(s):  
Stevie Marsden

As signifiers of literary value and taste, influencers of the literary canon, and indicators of distinction, literary prizes have played, and continue to play, an extremely important role in the promotion and celebration of literature. Far from being novel embellishments to an author’s career or book’s reputation, literary prizes have in fact become central components to the production, promotion, and longevity of literature in popular culture. They can increase book sales and print runs, heighten exposure and publicity, and consecrate an author’s place within literary canons. They are their own industry in and of themselves, their success dependent on many factors and agents including authors, publishers, booksellers, prize administrators, judges, and journalists. Literary prize scholarship is an ever-expanding, interdisciplinary field. Scholars have examined literary prizes in relation to cultural economics, sociology, linguistics, gender studies, postcolonial theory, book history, and publishing studies. However, when considering the impact of literary prize culture, it is important to remember that they are structured upon imperfect processes of judgment and selection. Yet, despite their limitations, literary prizes endure as one of the most captivating, dynamic and unique phenomena in literary and publishing culture. It is important for scholars to continue to interrogate literary prizes as a cultural phenomenon, in order to acquire a full understanding of the true impact they have on literary and publishing culture.


2019 ◽  
Vol 15 (4) ◽  
pp. 66-77
Author(s):  
Tetiana Yezhyzhanska ◽  
Tetiana Krainikova ◽  
Larysa Masimova

The impact of readers as target audiences of publishing houses in Ukraine on PR communication is not clearly understood. The goal of this research is to examine the role of readers in the communication process between publishing houses and customers. The readers become an important source of information about the events of the book publishing market and book novelties. The article shows the results of the poll of visitors of the largest book festivals in Ukraine – Book Arsenal Festival in Kyiv and Book Forum in Lviv for 2017–2019. These respondents (200 interviews per event) are not only the main consumers of book products publishing houses, but also they are the source of information about new books and activities of Ukrainian publishing houses themselves. According to the results of the poll, visitors of book fairs pay attention to the advice of their colleagues and friends, which are an important source of information about the events of the book publishing market and book novelties. Almost 50% of respondents create and distribute user-generated content about the events of the book publishing market. This activity is explained by the lack of information about the book market news of more than half of visitors. The results of the research confirm that readers are important publishing communications subjects, consumers are active advocates of the publisher’s brand, friends and colleagues actively create the content about the events of the book publishing market in Ukraine.


2021 ◽  
Vol 20 ◽  
pp. 895-937
Author(s):  
Martina Bečvářová ◽  
Stanisław Domoradzki

In the article, we will show the main important results of the international research project The impact of WWI on the formation and transformation of the scientific life of the mathematical community. It was supported by the Czech Science Foundation for the years 2018–2020 and brought together ten scientists from five countries (Czech Republic, Poland, Slovakia, USA, and Ukraine) and used the collaboration with historians of mathematics and mathematicians from many other European countries. We will discuss our motivation for the creation of the project, our methodological and professional preparations which profited from the international composition of the team and its longtime collaborations, profound specializations and experiences of the team members, and their deep and long-term studies of many archival sources and basic published works. We will present our choice of the general research trends, our definition of the scientific questions, and our determination of the main topics of our studies. We will describe our most important results (books, articles, visiting lectures, presentations at national and international conferences, seminars and book fairs, exhibitions, popularizations of the results between students, teachers, mathematicians, historians of sciences, and people who love mathematics and its history). We will analyze the new benefit that the project created for the future, for example, good platforms for future international research and cooperation, the discovery of many new interesting research questions, problems, and plans.


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.


Sign in / Sign up

Export Citation Format

Share Document