bluuebunny/crossref_metadata_2025_split huggingface dataset:
Un texte inédit : Kantemir (1708-1744) et la question de la langue
Authors: Breuillard Jean 
Published: January 2018

РезюМе
После смерти Петра i (1725) беспрецедентная коллективная работа начинается в России, в целях модернизации русской прозы. Этот проект будет завершен лишь в самом конце века. Среди тех выдающих писателей, которые приняли участие в этой многолетней работе первым по времени был Антиох Дмитриевич Кантемир (1708-1744), сын господаря Молдовы. Кантемир, желая «упростить » письменный язык, решил ввести в письменный язык слова из живого народного языка. Кантемир разделял сугубо лексическое представление языка. В этом отношении, он похож на Василия Тредиаковского (1703-1769), который в начале своей работы, также намеревался писать «просто » . Данное направление, в кото-ром привегирован парадигматика языка в ущерб синтагматике (взаимосвязи языковых единиц : синтаксис, ритм, анафора и т. д.) сделало возможным появле-ние блестящей поэзии. Тем не менее, в прозе дело обходилось иначе. В течение нескольких десятилетий проза оставалась слабым местом русской литературы, из-за отсутствия грамма тической мысли о синтаксисе и порядке слов. Лишен-ный стандартизированной прозы, полиглот Кантемир использовал несколько языков (феномен диглоссии или полиглоссии) в зависимости от жанра текста и личности получателя.
L’emploi des pronoms personnels en polonais (par contraste avec le russe et le français)
Authors: Włodarczyk Hélène 
Published: January 2018

Użycie zaimków osobowych w j. polskim (na tle j. rosyjskiego i w kontraście z francuskim)
tak w języku fr. jak i w j. polskim zaimki osobowe posiadają formy ortotoniczne i enklityczne. Jednakże użycie tych fom w obu tych językach jest różne, a gramatyki nie uwzględniają tego faktu przy pomocy jasnych reguł. W rodzinie języków słowiańskich j. polski znacznie różni sie od j. rosyjskiego ; bowiem wytworzyły się w nim nowe formy enklityczne zaimka w 3-ej osobie (go i mu), podczas gdy w j. rosyjskim formy enklityczne odziedziczone z prasłowiańszczyzny zanikły w j. współczesnym. Jednakże na nowszym etapie rozwoju j. polskiego jesteśmy świadkami nieprawidłowego używania form ortotonicznych i enklitycznych zaimka w 1-ej osobie (mi zamiast mnie). By wyjaśnić użycie tych dwóch rodzajów form przedstawianych w gramatykach jako warianty pozycyjne, opieram się na Meta-informacyjnej teorii centrów Uwagi (MIc – Meta-Informative centering theory), w której wypowiedzi podstawowe odróźniane są od rozszerzonych na podstawie ich metainformacyjnego statusu (datum/ novum). Form ortotonicznych używa się w wypowiedziach rozszerzonych, to znaczy w ekspresywnych wypowiedziach z punktu widzenia kontrastu między informacjami „ starą” (datum) a „ nową” (novum). Wreszcie kontrast ten pozwala na zdefiniowanie różnicy między topikiem a fokusem. W ramach teorii MIc stało się możliwe) systematyczne zestawienie użyć polskich form enklitycznych (pośród których należy odróżniać zerowe formy mianownika od elipsy podmiotu istniejącej w j. rosyjskim) z użyciami form enklitycznych w językach francuskim oraz rosyjskim, uwzględniając przy tym zagadnienie miejsca podmiotu zaimkowego w szyku wyrazów : przed lub po czasowniku. ogólnie rzecz biorąc używanie zaimków świadczy o tym, że pragmatyczne treści znajdują również bezpośrednie wykładniki zarówno w morfologii jak i składni.
La théorie de la langue chez Šiškov
Authors: Garde Paul 
Published: January 2018

Šiškov’s theory of language
In russian traditional historiography admiral a. s. Šiškov is viewed as a ridiculous figure, an enemy of progress who tries to promote an incomprehensible archaical language. But a thorough study of his writngs shows that whereas his famous book of 1803 against “ new style” is only a bad tempered libel, in the following years he wrote some well-thought-out texts where a real linguistic theory may be discovered. He insists on the difference between studies in language and in litterature, and states that the former should have an inductive method, on the basis of a systematic review of facts. He tries to define what is a language, and notes that it includes not only every day speech, but also special or dialectal items, as well as linguistic facts of the past, either known by documents or reconstructed. He calls his native language “ slavorussian”, and states that the so-called “ russian” and “ slavonic” (i. e. church slavonic) languages are one and the same, with only dialectal and stylistic differences, while all dialects and all styles are equally valuable. that language has also in his view a logical unity, since every language “ reasons in its own way”. the etymological link berween words is the reflection of the logical link between ideas, and the introduction of foreign words (by borrowing or by calque, which is still worse) can only disrupt that logic. this doctrine conveys some interesting and sound ideas. But its obvious shortcomings -dogmatism, negation of historical evolution, ignorance of the needs of present time – account for its failure.
Les « Français russes » à Moscou en 1812 : images de l’ennemi et destin d’une communauté d’émigrés
Authors: Rjéoutski Vladislav 
Published: January 2018

The “ Russian French” in Moscow in 1812 Images of the Enemy and Destiny of an Emigrant Community
This article deals with the question of the situation of French émigrés in Moscow before and during its occupation by the Napoleonic army. The Russian government, some social groups and Moscow authorities built the image of an interior enemy and it complicated the conditions of life of the French community in Moscow. During the occupation, some French people were involved in the municipality created by the occupational authorities in Moscow. However, only a few of them were sentenced after Moscow was liberated by the Russian army.
Inciderunt itaque in fossam quam sibi ipsi fecerunt : Mass Grave of Napoleon’s Soldiers in Vilnius, December 1812 [Inciderunt itaque in fossam quam sibi ipsi fecerunt : La fosse commune des soldats de Napoléon à Vilnius, décembre 1812]
Authors: Jankauskas Rimantas 
Published: January 2018

Inciderunt itaque in fossam quam sibi ipsi fecerunt
Братская могила солдат Наполеона в Вильнюсе, декабрь 1812 г.
Вскрытие этой братской могилы с целью ее спасения от разрушения, имело место весной и в сентябре 2012 г. Оно позволило обследовать поверхность примерно в
600 м2. В могиле было обнаружено
3269 человек, в основном мужчин, но так-же несколько женщин. Возраст и сложение соответствуют требованиям, предъявляв-шимся при наборе во французскую армию. Анализ патологий выявил немногочислен-ные травмы. Незалеченные травмы были, возможно, вызваны грубым обращением с телами при их захоронении. Были выявле-ны следы 34 леченных травм, переломы длинных костей хорошо срослись, что под-тверждает высокую квалификацию хирур-гов и/ или хороший подбор новобранцев. Было отмечено несколько случаев патоло-гий, характерных для солдат, подверг-шихся большим нагрузкам (в особенности в пехоте) : 8 случаев болезни Шейерманна
(поражение кости позвоночника) и 6 слу-чаев «маршевой стопы » (перелом во время переходов). По крайней мере 3 не пол-ностью залеченные травмы могли иметь причиной свежие ранения, произошедшие во время этой кампании. Было также отме-чено несколько следов инфекционных забо-леваний, как специфических (таких как третичный сифилис или риккетсиозы), так и неспецифических, а также случаи раз-личных изменений полости рта и обычных изменений костей и зубов.
Une lettre inédite de Herzen à Charles Edmond, et de celui-ci à Proudhon. Publication, commentaires et notes
Authors: Desurvire Emmanuel , Mervaud Michel 
Published: January 2018

An Unpublished Letter from Herzen to Charles Edmond and Another One of Charles Edmond to Proudhon
In early December 1852, Herzen learnt that Charles Edmond’s young daughter was probably in Paris with his own daughters at Maria Reichel’s home. In this previously unpublished letter, he announces his wish to go to Paris to meet his daughters again. Moreover, he is impatient to get an answer from Proudhon, whom he apparently admires a lot. Charles Edmond transmits Herzen’s letter to Proudhon, and in his, also unpublished letter, considers that Herzen is flattering Proudhon too much.
А. В. Дружинин : «… видеть Францию мне было полезно очень» : Париж 1857 года глазами русского путешественника. Publication, commentaires et notes. [A. V. Družinin : “… visiting France has been very helpful for me” : Paris in 1857 as Described by a Russian Traveller]
Authors: Aldonina N. B. 
Published: January 2018

A. V. Družinin : “… visiting France has been very helpful for me” Paris in 1857 as Described by a Russian Traveller
On the basis of archives, the article goes back over the stay in Paris of the Russian writer and critic A. V. Družinin (1824-1864) during summer 1857. Every detail has been noted : the places he visited, the kind of occupations he had, the people he met. Družinin’s observations on nature in France, on its social and artistic life will be related in a series of documents written in the 1860’ s. All the facts mentioned here from a scientific point of view are interesting for the study of the biography of the author, but also for a broader analysis of the cultural relations between France and Russia.
Producing Distant Planets by Mutual Scattering of Planetary Embryos
Authors: Silsbee Kedron , Tremaine Scott 
Published: January 2018

Abstract
It is likely that multiple bodies with masses between those of Mars and Earth (“planetary embryos”) formed in the outer planetesimal disk of the solar system. Some of these were likely scattered by the giant planets into orbits with semimajor axes of hundreds of au. Mutual torques between these embryos may lift the perihelia of some of them beyond the orbit of Neptune, where they are no longer perturbed by the giant planets, so their semimajor axes are frozen in place. We conduct N-body simulations of this process and its effect on smaller planetesimals in the region of the giant planets and the Kuiper Belt. We find that (i) there is a significant possibility that one sub-Earth mass embryo, or possibly more, is still present in the outer solar system; (ii) the orbit of the surviving embryo(s) typically has perihelion of 40–70 au, semimajor axis less than 200 au, and inclination less than 30°; (iii) it is likely that any surviving embryos could be detected by current or planned optical surveys or have a significant effect on solar system ephemerides; (iv) whether or not an embryo has survived to the present day, its dynamical influence earlier in the history of the solar system can explain the properties of the detached disk (defined in this paper as containing objects with perihelia >38 au and semimajor axes between 80 and 500 au).
Transiting Exoplanet Monitoring Project (TEMP). III. On the Relocation of the Kepler-9 b Transit
Authors: Wang Songhu , Wu Dong-Hong , Addison Brett C. , Laughlin Gregory , Liu Hui-Gen , Wang Yong-Hao , Yang Taozhi , Yang Ming , Yisikandeer Abudusaimaitijiang , Hong Renquan , Li Bin , Liu Jinzhong , Zhao Haibin , Wu Zhen-Yu , Hu Shao-Ming , Zhou Xu , Zhou Ji-Lin , Zhang Hui , Zheng Jie , Wang Wei , Fan Zhou , Niu Hubiao , Chen Yuan-Yuan , Lu Hao , Peng Xiyan , Li Kai , Guo Di-Fu 
Published: January 2018

AbstractThe Kepler-9 system harbors three known transiting planets. The system holds significant interest for several reasons. First, the outer two planets exhibit a period ratio that is close to a 2:1 orbital commensurability, with attendant dynamical consequences. Second, both planets lie in the planetary mass “desert” that is generally associated with the rapid gas agglomeration phase of the core accretion process. Third, there exist attractive prospects for accurately measuring both the sky-projected stellar spin–orbit angles as well as the mutual orbital inclination between the planets in the system. Following the originalKeplerdetection announcement in 2010, the initially reported orbital ephemerides for Kepler-9 b and c have degraded significantly, due to the limited time base-line of observations on which the discovery of the system rested. Here, we report new ground-based photometric observations and extensive dynamical modeling of the system. These efforts allow us to photometrically recover the transit of Kepler-9 b and thereby greatly improve the predictions for upcoming transit mid-times. Accurate ephemerides of this system are important in order to confidently schedule follow-up observations of this system, for both in-transit Doppler measurements as well as for atmospheric transmission spectra taken during transit.
Quiescent Prominences in the Era of ALMA. II. Kinetic Temperature Diagnostics
Authors: Gunár Stanislav , Heinzel Petr , Anzer Ulrich , Mackay Duncan H. 
Published: January 2018

Abstract
We provide the theoretical background for diagnostics of the thermal properties of solar prominences observed by the Atacama Large Millimeter/submillimeter Array (ALMA). To do this, we employ the 3D Whole-Prominence Fine Structure (WPFS) model that produces synthetic ALMA-like observations of a complex simulated prominence. We use synthetic observations derived at two different submillimeter/millimeter (SMM) wavelengths—one at a wavelength at which the simulated prominence is completely optically thin and another at a wavelength at which a significant portion of the simulated prominence is optically thick—as if these were the actual ALMA observations. This allows us to develop a technique for an analysis of the prominence plasma thermal properties from such a pair of simultaneous high-resolution ALMA observations. The 3D WPFS model also provides detailed information about the distribution of the kinetic temperature and the optical thickness along any line of sight. We can thus assess whether the measure of the kinetic temperature derived from observations accurately represents the actual kinetic temperature properties of the observed plasma. We demonstrate here that in a given pixel the optical thickness at the wavelength at which the prominence plasma is optically thick needs to be above unity or even larger to achieve a sufficient accuracy of the derived information about the kinetic temperature of the analyzed plasma. Information about the optical thickness cannot be directly discerned from observations at the SMM wavelengths alone. However, we show that a criterion that can identify those pixels in which the derived kinetic temperature values correspond well to the actual thermal properties in which the observed prominence can be established.
Blazar Sheath Illumination of the Outer Molecular Torus: A Resolution of the Seed Photon Problem for the Far-GeV Blazar Flares
Authors: Breiding Peter , Georganopoulos Markos , Meyer Eileen T. 
Published: January 2018

Abstract
Recent multiwavelength work led by the Boston University blazar group (e.g., Marscher et al.) strongly suggests that a fraction of the blazar flares seen by the Fermi Large Area Telescope (LAT) take place a few to several pc away from the central engine. However, at such distances from the central engine, there is no adequate external photon field to provide the seed photons required for producing the observed GeV emission under leptonic inverse Compton (IC) models. A possible solution is a spine-sheath geometry for the emitting region (MacDonald et al., but see Nalewajko et al.). Here we use the current view of the molecular torus (e.g., Elitzur; Netzer), in which the torus extends a few pc beyond the dust sublimation radius with dust clouds distributed with a declining density for decreasing polar angle. We show that for a spine-sheath blazar jet embedded in the torus, the wide beaming pattern of the synchrotron radiation of the relatively slow sheath will heat molecular clouds with subsequent IR radiation that will be highly boosted in the spine comoving frame, and that under reasonable conditions this photon field can dominate over the sheath photons directly entering the spine. If the sheath is sufficiently luminous it will sublimate the dust, and if the sheath synchrotron radiation extends to optical-UV energies (as may happen during flares), this will illuminate the sublimated dust clouds to produce emission lines that will vary in unison with the optical-UV continuum, as has been very recently reported for blazar CTA 102 (Jorstad et al.).
Radiation Transfer of Models of Massive Star Formation. IV. The Model Grid and Spectral Energy Distribution Fitting
Authors: Zhang Yichen , Tan Jonathan C. 
Published: January 2018

Abstract
We present a continuum radiative transfer model grid for fitting observed spectral energy distributions (SEDs) of massive protostars. The model grid is based on the paradigm of core accretion theory for massive star formation with pre-assembled gravitationally bound cores as initial conditions. In particular, following the turbulent core model, initial core properties are set primarily by their mass and the pressure of their ambient clump. We then model the evolution of the protostar and its surround structures in a self-consistent way. The model grid contains about 9000 SEDs with four free parameters: initial core mass, the mean surface density of the environment, the protostellar mass, and the inclination. The model grid is used to fit observed SEDs via

minimization, with the foreground extinction additionally estimated. We demonstrate the fitting process and results using the example of massive protostar G35.20-0.74. Compared with other SED model grids currently used for massive star formation studies, the properties of the protostar and its surrounding structures are more physically connected in our model grid, which reduces the dimensionality of the parameter spaces and the total number of models. This excludes possible fitting of models that are physically unrealistic or are not internally self-consistent in the context of the turbulent core model. Thus, this model grid serves not only as a fitting tool to estimate properties of massive protostars, but also as a test of core accretion theory. The SED model grid is publicly released with this paper.
All-flavor Search for a Diffuse Flux of Cosmic Neutrinos with Nine Years of ANTARES Data
Authors: Albert A. , André M. , Anghinolfi M. , Anton G. , Ardid M. , Aubert J.-J. , Aublin J. , Avgitas T. , Baret B. , Barrios-Martí J. , Basa S. , Belhorma B. , Bertin V. , Biagi S. , Bormuth R. , Bourret S. , Bouwhuis M. C. , Brânzaş H. , Bruijn R. , Brunner J. , Busto J. , Capone A. , Caramete L. , Carr J. , Celli S. , El Moursli R. Cherkaoui , Chiarusi T. , Circella M. , Coelho J. A. B. , Coleiro A. , Coniglione R. , Costantini H. , Coyle P. , Creusot A. , Díaz A. F. , Deschamps A. , Bonis G. De , Distefano C. , Palma I. Di , Domi A. , Donzaud C. , Dornic D. , Drouhin D. , Eberl T. , Bojaddaini I. El , Khayati N. El , Elsässer D. , Enzenhöfer A. , Ettahiri A. , Fassi F. , Felis I. , Fusco L. A. , Gay P. , Giordano V. , Glotin H. , Grégoire T. , Ruiz R. Gracia , Graf K. , Hallmann S. , Haren H. van , Heijboer A. J. , Hello Y. , Hernández-Rey J. J. , Hößl J. , Hofestädt J. , Illuminati G. , James C. W. , Jong M. de , Jongen M. , Kadler M. , Kalekin O. , Katz U. , Kießling D. , Kouchner A. , Kreter M. , Kreykenbohm I. , Kulikovskiy V. , Lachaud C. , Lahmann R. , Lefèvre D. , Leonora E. , Lotze M. , Loucatos S. , Marcelin M. , Margiotta A. , Marinelli A. , Martínez-Mora J. A. , Mele R. , Melis K. , Michael T. , Migliozzi P. , Moussa A. , Navas S. , Nezri E. , Organokov M. , Păvălaş G. E. , Pellegrino C. , Perrina C. , Piattelli P. , Popa V. , Pradier T. , Quinn L. , Racca C. , Riccobene G. , Sánchez-Losa A. , Saldaña M. , Salvadori I. , Samtleben D. F. E. , Sanguineti M. , Sapienza P. , Schüssler F. , Sieger C. , Spurio M. , Stolarczyk Th. , Taiuti M. , Tayalati Y. , Trovato A. , Turpin D. , Tönnis C. , Vallage B. , Elewyck V. Van , Versari F. , Vivolo D. , Vizzoca A. , Wilms J. , Zornoza J. D. , Zúñiga J. ,   (The ANTARES Collaboration)
Published: January 2018

Abstract
The ANTARES detector is at present the most sensitive neutrino telescope in the northern hemisphere. The highly significant cosmic neutrino excess observed by the Antarctic IceCube detector can be studied with ANTARES, exploiting its complementing field of view, exposure, and lower energy threshold. Searches for an all-flavor diffuse neutrino signal, covering nine years of ANTARES data taking, are presented in this Letter. Upward-going events are used to reduce the atmospheric muon background. This work includes for the first time in ANTARES both track-like (mainly

and shower-like (mainly

) events in this kind of analysis. Track-like events allow for an increase of the effective volume of the detector thanks to the long path traveled by muons in rock and/or sea water. Shower-like events are well reconstructed only when the neutrino interaction vertex is close to, or inside, the instrumented volume. A mild excess of high-energy events over the expected background is observed in nine years of ANTARES data in both samples. The best fit for a single power-law cosmic neutrino spectrum, in terms of per-flavor flux at 100 TeV, is

10−18 GeV−1 cm−2 s−1 sr−1 with spectral index

. The null cosmic flux assumption is rejected with a significance of 1.6σ.
A Patient with Multiple Keratinocytic Cancers (MKC): Uncommon Presentation in a Bulgarian Patient
Authors: Tchernev Georgi , Philipov Stanislav , Chokoeva Anastasiya Atanasova , Wollina Uwe , Lotti Torello , Lozev Ilia , Yungareva Irina , Maximov Georgi Konstantinov 
Published: January 2018

Keratinocyte skin cancers, including basal cell carcinoma (BCC) and squamous cell carcinoma (SCC), are the most common cancer occurring in people with fair skin, worldwide. Despite all known triggers, several suggested contributors are still investigated. We will focus our attention on the personal history of previous cancers and radiation exposure as occupational risk factors, as in the presented case. We report a patient, with multiple BCCs, and subsequent occurrence of a SCC on photo-exposed area of the face, as we want to emphasize the importance of strict following up of these patients, regarding the risk for developing new tumors in short periods of time, no matter if the triggering exposure factor is known from the history, or not. Although keratinocytes tumours are associated with the low mortality rate, we focus the attention on the fact, that the history of non-melanoma skin cancer is associated with increased mortality.
Peri - and Intraocular Mutilating Advanced Squamous Cell Carcinoma: ʺMonsters Inside Your Bodyʺ?
Authors: Tchernev Georgi , Lotti Torello , Lozev Ilia , Maximov Georgi Konstantinov , Wollina Uwe 
Published: January 2018

Periocular malignancies represent between 5% and 10% of all types of skin cancers. The incidence of eyelid (but also the periocular located) malignancies seems to differ in distribution across the continents. The incidence of eyelid tumours (but also the periocular located tumours) in a predominantly white population determined that BCC is the most common malignant periocular eyelid tumour in whites. This finding has been replicated consistently throughout the literature, with BCC representing 85–95% of all eyelid malignancies, SCC representing 3.4 - 12.6%, Seb Ca representing 0.6 - 10.2%, and both melanoma and Merkel cell carcinoma representing less than 1%. Most periocular skin cancers are associated with ultraviolet radiation (UVR) exposure. Ultraviolet radiation causes local immune suppression, which, coupled with DNA abnormalities in tumour suppressor genes and oncogenes, leads to the development of skin cancers. We are presenting a 62 - year - old patient with a small nodule about 2 cm away from the lower lid of his left eye. A tumour was surgically treated. Several years later there was a tumour relapse, treated with radiotherapy and subsequent chemotherapy with Endoxan and Cisplatin. After the second relapse, he was treated surgically in general anaesthesia by orbital exenteration, removal of the orbital floor and resection of zygomatic bone and the maxillary sinus. A couple of months later, he developed a tumour relapse in the scars and the area of a primary tumour with tumour progression. A possible therapy with Cetuximab or radiation therapy was discussed as a possible treatment option.