bluuebunny/crossref_metadata_2025_split huggingface dataset:
Neuroinflammation and Epileptogenesis (Literature Review)
Authors: Зайцев И.И. , Лихачев С.А. , Куликова С.Л. , Севосей И.Д. , Мелик-Касумов Т.Б. 
Published: February 2022

Эпилептология является одним из наиболее актуальных направлений в современной неврологии. Эпилепсия наносит значительный урон ментальному и физическому здоровью человека, повышает риск преждевременной смерти, существенно ухудшает качество жизни пациента и его семьи, а также повышает финансовую нагрузку на систему здравоохранения. Вышесказанным продиктована потребность дальнейшего изучения фундаментальных процессов, обусловливающих развитие и поддержание эпилепсии. За последние десятилетия появились исследования, свидетельствующие о связи нейровоспаления и эпилептогенеза. Ключевым субстратом концепции нейровоспаления выступает дисбаланс между воспалительными и противовоспалительными цитокинами. В данной статье дано подробное описание воздействия воспалительных (интерлейкин-1, -2, -6, -8 и фактор некроза опухолей альфа) и противовоспалительных цитокинов (антагонист рецептора интерлейкина-1, интерлейкин-4, -10) на функциональное состояние нейронов. В обзоре литературы приведены результаты изучения нейровоспаления на клеточных препаратах и животных моделях, а также исследований, посвященных изучению влияния цитокинов на эпилепсию у людей.
Epileptology is one of the most relevant areas in modern neurology. Epilepsy causes significant damage to the mental and physical health of a person, increases the risk of premature death, significantly worsens the quality of life of the patient and their family, as well as increases the financial burden on the health care system. This causes the need for further study of the fundamental processes that determine the development and maintenance of epilepsy. Over the past decades, there have been studies that suggest the connection between neuroinflammation and epileptogenesis. The key substrate of the concept of neuroinflammation is the imbalance between inflammatory and anti-inflammatory cytokines. This article provides a detailed description of the effects of inflammatory (interleukin-1, interleukin-2, interleukin-6, interleukin-8, and tumor necrosis factor alpha) and anti-inflammatory cytokines (interleukin-1 receptor antagonist, interleukin-4, interleukin-10) on the functional state of neurons. The literature review presents the results of the study of neuroinflammation in cellular preparations and animal models, as well as the results of the studies on the effect of cytokines on epilepsy in humans.
Possibility of Using L-Carnitine in Patients with COVID-Associated Liver Damage
Authors: Одинец Д.Ф. , Литвинович С.Н. , Дорошкевич И.П. , Капитонова Е.И. 
Published: February 2022

Внастоящее время инфекция SARS-CoV-2 является одним из самых распространенных заболеваний в мире, приводящим к ухудшению качества жизни, инвалидизации и многочисленным летальным исходам. Наряду с поражением легких, у пациентов отмечается частое вовлечение в воспалительный процесс других органов и систем, в том числе и печени. Целью данной статьи является определение возможности использования L-карнитина в лечении поражения печени, ассоциированного с SARS-CoV-2.
Nowadays, SARS-CoV-2 infection is one of the most common diseases in the world, which leads to deterioration of the quality of life, disability, and numerous deaths. Along with damage to the lungs, patients have frequent involvement of other organs and systems in the inflammatory process, including liver. The purpose of this article is to determine the possibility of using L-carnitine in the treatment of liver damage associated with SARS-COV-2.
Preparations of Soluble Platelet Factors - New Options of Regenerative Medicine
Authors: Потапнёв М.П. , Богдан В.Г. , Кривенко С.И. , Янушко В.Я. , Панченко М.А. , Кондратенко Г.Г. , Неверов П.С. , Федоренко С.В. , Загородный Г.М. , Ясюкевич А.С. , Гулевич Н.П. , Космачева С.М. , Асаевич В.И. , Лицкевич П.В. , Эйсмонт О.Л. , Букач Д.В. , Троянов А.А. , Игнатенко С.И. 
Published: February 2022

В кратком обзоре дано представление о препаратах растворимых факторов тромбоцитов (РФТ) человека и их медицинском применении. Отмечено, что препараты РФТ уже широко используются для лечения длительно заживающих ран кожи и слизистых, а также при травмах и заболеваниях опорно-двигательного аппарата. Существуют области медицины, в которых активно изучаются условия для успешного местного применения препаратов РФТ: клеточная терапия, пластическая хирургия, офтальмология, кожные болезни, косметология, офтальмология, акушерство и гинекология, неврология. Сделан вывод о целесообразности дальнейшего медицинского изучения показаний для эффективного применения препаратов РФТ.
A brief review provides the data on the preparations of human soluble platelet factors (SPF) and their medical use. It is noted that SPF preparations are widely used for the treatment of long-term healing wounds of the skin and mucous membranes, as well as for injuries and diseases of the musculoskeletal system. There are the areas of medicine, where the conditions for successful topical use of SPF are being actively studied. These are the cell therapy, plastic surgery, ophthalmology, skin diseases, cosmetology, obstetrics and gynecology, neurology. The conclusion is made about the expediency of further medical study of the indications for the effective use of SPF preparations.
Determinantes de compra del consumidor de prendas de vestir en la provincia de Tungurahua
Authors: Molina Arcos Ibeth Aracelly , Tamayo Viera Jorge Oswaldo , Pérez Yauli Vicente Leonardo , Arroba Freire Edison Manuel 
Published: February 2022

La presente investigación se centra en el estudio del comportamiento del consumidor, en relación a las diferentes prendas de vestir confeccionadas. El objetivo fue identificar y categorizar los factores que determinan el consumo de prendas confeccionadas y el comportamiento de compra en la ciudad de Ambato – provincia de Tungurahua, Ecuador.
El estudio presenta los resultados proporcionados por un modelo de investigación descriptiva con determinantes clave para la compra de prendas confeccionadas que se pueden agrupar en las categorías, (1) estilo de vida, (2) liderazgo de moda, (3) atributos económicos, y (4) contexto de consumo. La revisión ofrece una visión general sistemática del diverso conjunto de conceptos y orientaciones que se han utilizado, hasta ahora, para examinar el comportamiento de los consumidores hacia la compra de prendas confeccionadas. Los hallazgos muestran que existe un fuerte enfoque en la sostenibilidad de la ropa. El consumo sustentable ha originado el impulso de investigaciones que procuran develar tácticas que admitan la concienciación de las corresponsabilidades sociales, frente a la decisión de compra, tanto desde la perspectiva de consumidor, productor como del comerciante. El análisis se realizó a través de criterios de evaluación, aglutinando a la mayoría de los consumidores en prendas confeccionadas, productores y comerciantes.
EFL Learners’ Self Efficacy and Its Relation to Reading Comprehension in Online Learning
Authors: Tarigan Fatin Nadifa , Hasibuan Siti Aminah , Damanik Lia Agustina , Tambunan Rika Wahyuni 
Published: February 2022

Self-efficacy plays an influential role in iniating any action including reading especially in online learning. Reading comprehension, along with all other language skills, has become a big concern in ELT, while self-efficacy is a pyschological aspect that affect the learners’ success in mastering the skill. In this regard, this study attempts to find out whether EFL learners’ self-efficacy affects the learners’ reading comprehension in Universitas Pembinaan Masyarakat Indonesia. The study applied correctional study with quantitative design. Participants in this study were 50 learners of English Education Department. A self-efficacy questionnaire (SEQ) and reading comprehension test were applied to the participants as parts of the correlational research model. The collected quantitative data were analyzed by Statistical Package for the Social Sciences (SPSS) program. The finding shows that the result of r-calculation for learners’ self-efficacy and their reading score is .765. The score of significance level is < 0.05 (0.000 < 0.05) which means that Ha was accepted and H0 was rejected. This score indicates that there is a positive correlation between the two variables.
Il calo della partecipazione elettorale nelle elezioni amministrative in Norvegia
Authors: Bjørklund Tor 
Published: February 2022

Il declino della partecipazione elettorale: fenomeno diffuso e caso norvegese. Prospettive di analisi per le elezioni amministrative.
Le cause.
Le conseguenze.
Tasso di partecipazione elettorale e partecipazione politica monotematica.
Ricapitolazione.
L'elaborazione della cosiddetta ‘legge truffa’ e le elezioni del 1953
Authors: Possanzini Davide 
Published: February 2022

Le elezioni amministrative del 1951 e del 1952 e la crisi del centrismo.
Perché la legge: la scelta del premio maggioritario.
Il disegno di legge Scelba.
L'ostruzionismo parlamentare delle opposizioni.
La campagna elettorale e le liste laiche dissidenti.
I risultati elettorali e la fine del centrismo.
Istituzioni politiche e processi elettorali in Marocco
Authors: Montabes Pereira Juan , Parejo Fernandez Maria Angustias 
Published: February 2022

Una monarchia costituzionale solo di facciata.
Il ruolo delle elezioni nel sistema politico marocchino.
I partiti.
I processi elettorali fino al 1996.
Il sistema elettorale dopo la riforma costituzionale.
I risultati elettorali dal 1963 al 1997.
PELATIHAN PEMBUATAN VIDEO PEMBELAJARAN UNTUK GURU SMA KALAM KUDUS
Authors: Anggraini Lya Dewi , Dewi Yuli Kartika , Sutrisno Timotius Febry Christian Wahyu 
Published: February 2022

Pembelajaran daring menjadi satu-satunya pilihan yang dapat dilakukan semasa pandemi, namun tantangan yang dihadapi adalah bagaimana pembelajaran tersebut mampu terlaksana dengan lebih menarik bagi para siswa berbasis kreativitas, inovasi, dan penciptaan nilai tambah sebagai bentuk entrepreneurial activity. Keterbatasan para guru dalam pemanfaatan teknologi diatasi dengan pelatihan pembuatan video pembelajaran yang interaktif. Kegiatan ini dilaksanakan sepenuhnya secara daring antara tim Universitas Ciputra dengan kepala sekolah dan para guru SMAK Kalam Kudus Surabaya. Tujuan utamanya adalah untuk meningkatkan pengetahuan dan kemampuan para guru terhadap teknologi informasi yang berguna untuk pembuatan dan pengeditan video secara praktis. Metode yang digunakan adalah diskusi interaktif tentang kondisi aktual yang dihadapi di lapangan, identifikasi pengetahuan dan kemampuan para guru, jenis mata pelajaran, dan pengamatan kondisi fisik di lapangan untuk melihat ketersediaan sarana prasarana. Selama pelatihan, ketertarikan dan minat para guru meningkat cukup tinggi dari banyaknya pertanyaan yang diajukan. Hal ini menimbulkan kebutuhan untuk penyusunan rencana pembelajaran secara daring, sebelum video pembelajaran yang menarik dapat dibuat. Tantangan waktu operasional sekolah yang sangat terbatas tidak menyurutkan keinginan para guru untuk mengatur dan mempersiapkan strategi pembelajaran yang lebih sistematis dan terencana terutama untuk mengantisipasi waktu yang lebih panjang saat pengeditan video.
Movement, Feeding Behaviour and Threats of Colobus guereza Ruppellin at Seasonally Dry Riverine Forest of Engare-Olmotonyi and Arboreta of the Forestry Training Institute’s Olmotonyi’s Campus in Northern Highlands of Tanzania
Authors: Kayombo Canisius John , Kivuyo Tumaini , Giliba Richard A. , Kyando Sefania J. , Lugumira Emmanuel , Gwau Hussein Said 
Published: February 2022

The observation of feeding and movement behaviour of wild fauna is significant in the process of understanding the ecosystems. The movement and feeding behaviour of An assessment on the movement, feeding behaviour, and threats of Colobus guereza was done in Engare-olmotonyi seasonally dry riverine forest and arboreta at the Forestry Training Institutes-Olmotonyi in northern Tanzania. The movement and feeding behaviour were monitored for 30 days from mid of September to October 2020. Sleeping and waking up times, trees fed by C. guereza, and trees they slept on were recorded and estimated for their height and canopy cover (light or dense). The human threats were also recorded. The findings revealed that C. Guereza members were waking up between 6.30 am and 6.58 am, depending on the condition of the sky (clear or cloudy). When the sky was clear they wake up between 6.30 and 6.45 am, and 6.45 am to 6.58 am on cloudy sky days. They slept on the highest canopy trees and were feeding on tender or mature leaves depending on the type of species. The flowers and fruits of Jacaranda mimosifolia, Albizia gummifera (J.F.Gmel.) C.A.Sm., Cussonia holstii Harms ex Engl and leaves of Lagenaria abyssinica (Hook.fil.) C.Jeffrey were found to be fed by C. guereza. As soon as they wake up, they both of them urinated. Then, young C. guereza were found to be directed to move before adults just after they had urinated. The height of trees the C. guereza were found to jump on and or sleep ranged from 24 ± 10 m, with an average height of 17 m. The tallest trees ranged from a height of 24 ± 20 m; while the medium had a height of ≤ 20 ± ≤15 m. Most of the tallest trees were Albizia gummifera (J.F.Gmel.) C.A.Sm., Jacaranda mimosifolia D.Don; Cussonia holstii Harms ex Engl.; and Eucalptys maidenii F. Muell. The threats to C. guereza were cutting of trees as their food and habitat and illegal routes that disturbed their behaviour of feeding and movement. The direction of C. guereza movements and sleeping depend most on the trees. Further study is needed to evaluate the plant species being fed at different seasons, protect the existing trees, and restore the forest gaps.
Online Database of Multiwavelength Water Masers in Galactic Star-forming Regions
Authors: Ladeyschikov Dmitry A. , Sobolev Andrey M. , Bayandina Olga S. , Shakhvorostova Nadezhda N. 
Published: February 2022

Abstract
In this paper, we present an online multiwavelength database of water masers in star-forming regions of the Galaxy. The collected data represent ∼95% of all observations of water masers in star-forming regions published since 1989. Nineteen transitions are included, from 22 GHz to 1.88 THz. The MaserDB.net information system provides fast and open access to the collected data, including maser tabular data, spectra, and interferometric maser spot data. The database covers ∼18,700 individual observations and ∼7200 maser detections. The data on the water maser detection are available for ∼2600 sources, and interferometric data are available for ∼560 sources. Statistical analysis of the water masers’ data and comparison with other abundant maser species found in star-forming regions (OH and CH3OH of class I and II) show that water masers are the most ubiquitous maser type. Access to the water maser database is available online at https://MaserDB.net. The database can be queried using a web search form or Structured Query Language.
Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
Authors: Kilpatrick Charles D. , Fong Wen-fai , Blanchard Peter K. , Leja Joel , Nugent Anya E. , Palmese Antonella , Paterson Kerry , Starkenburg Tjitske , Alexander Kate D. , Berger Edo , Chornock Ryan , Hajela Aprajita , Margutti Raffaella 
Published: February 2022

Abstract
We present the complete set of Hubble Space Telescope imaging of the binary neutron star merger GW170817 and its optical counterpart AT 2017gfo. Including deep template imaging in F814W, F110W, F140W, and F160W at 3.4 yr post-merger, we reanalyze the full light curve of AT 2017gfo across 12 bands from 5 to 1273 rest-frame days after merger. We obtain four new detections of the short γ-ray burst 170817A afterglow from 109 to 170 rest-frame days post-merger. These detections are consistent with the previously observed β = −0.6 spectral index in the afterglow light curve with no evidence for spectral evolution. We also analyze our limits in the context of kilonova afterglow or IR dust echo emission but find that our limits are not constraining for these models. We use the new data to construct deep optical and IR stacks, reaching limits of M = −6.3 to −4.6 mag, to analyze the local environment around AT 2017gfo and low surface brightness features in its host galaxy NGC 4993. We rule out the presence of any globular cluster at the position of AT 2017gfo to 2.3 × 104
L
⊙, including those with the reddest V − H colors. Finally, we analyze the substructure of NGC 4993 in deep residual imaging and find shell features that extend up to 71.″8 (14.2 kpc) from NGC 4993. The shells have a cumulative stellar mass of 6.3 × 108
M
⊙, roughly 2% of NGC 4993, and mass-weighted ages of >3 Gyr. We conclude that it was unlikely that the GW170817 progenitor system formed in the galaxy merger.
Stars Crushed by Black Holes. II. A Physical Model of Adiabatic Compression and Shock Formation in Tidal Disruption Events
Authors: Coughlin Eric R. , Nixon C. J. 
Published: February 2022

Abstract
We develop a Newtonian model of a deep tidal disruption event (TDE), for which the pericenter distance of the star, r
p, is well within the tidal radius of the black hole, r
t, i.e., when β ≡ r
t/r
p ≫ 1. We find that shocks form for β ≳ 3, but they are weak (with Mach numbers ∼1) for all β, and that they reach the center of the star prior to the time of maximum adiabatic compression for β ≳ 10. The maximum density and temperature reached during the TDE follow much shallower relations with β than the previously predicted

ρ

max

∝

β

3

and

T

max

∝

β

2

scalings. Below β ≃ 10, this shallower dependence occurs because the pressure gradient is dynamically significant before the pressure is comparable to the ram pressure of the free-falling gas, while above β ≃ 10, we find that shocks prematurely halt the compression and yield the scalings

ρ

max

∝

β

1.62

and

T

max

∝

β

1.12

. We find excellent agreement between our results and high-resolution simulations. Our results demonstrate that, in the Newtonian limit, the compression experienced by the star is completely independent of the mass of the black hole. We discuss our results in the context of existing (affine) models, polytropic versus non-polytropic stars, and general relativistic effects, which become important when the pericenter of the star nears the direct capture radius, at β ∼ 12.5 (2.7) for a solar-like star disrupted by a 106
M
⊙ (107
M
⊙) supermassive black hole.
Dynamical Friction and Tidal Interactions
Authors: Roshan Mahmood , Mashhoon Bahram 
Published: February 2022

Abstract
We discuss dynamical friction in an N-body system in the presence of tidal interactions caused by a distant external source. Using the distant tide approximation, we develop a perturbation scheme for the calculation of dynamical friction that takes tidal effects into account in linear order. In this initial analytic approach to the problem, we neglect the influence of tides on the distribution function of stars in the background stellar system. Our result for the dynamical friction force in the appropriate limit is in agreement with Chandrasekhar’s formula in the absence of tides. We provide preliminary estimates for the tidal contributions to the dynamical friction force. The astrophysical implications of our results are briefly discussed.
The Critical Core Mass of Rotating Planets
Authors: Zhong Wei , Yu Cong 
Published: February 2022

Abstract
The gravitational harmonics measured from the Juno and Cassini spacecraft help us specify the internal structure and chemical elements of Jupiter and Saturn, respectively. However, we still do not know much about the impact of rotation on the planetary internal structure as well as on their formation. The centrifugal force induced by the rotation deforms the planetary shape and partially counteracts the gravitational force. Thus, rotation will affect the critical core mass of the exoplanet. Once the atmospheric mass becomes comparable to the critical core mass, the planet will enter the runaway accretion phase and become a gas giant. We have confirmed that the critical core masses of rotating planets depend on the stiffness of the polytrope, the outer boundary conditions, and the thickness of the isothermal layer. The critical core mass with the Bondi boundary condition is determined by the surface properties. The critical core mass of a rotating planet will increase with the core gravity (i.e., the innermost density). For the Hill boundary condition, the soft polytrope shares the same properties as planets with the Bondi boundary condition. Because the total mass for planets with the Hill boundary condition increases with the decrease of the polytropic index, a higher core gravity is required for rotating planets. As a result, the critical core mass in the stiff Hill model sharply increases. The rotational effects become more important when the radiative and convective regions coexist. Further, the critical core mass of planets with the Hill (Bondi) boundary increases noticeably as the radiative layer becomes thinner (thicker).
Synchronization of Small-scale Magnetic Features, Blinkers, and Coronal Bright Points
Authors: Shokri Zahra , Alipour Nasibe , Safari Hossein , Kayshap Pradeep , Podladchikova Olena , Nigro Giuseppina , Tripathi Durgesh 
Published: February 2022

Abstract
We investigate the relationship between different transients such as blinkers detected in images taken at 304 Å, extreme ultraviolet coronal bright points (ECBPs) at 193 Å, X-ray coronal bright points (XCBPs) at 94 Å on the Atmospheric Imaging Assembly, and magnetic features observed by the Helioseismic and Magnetic Imager during 10 yr of solar cycle 24. An automatic identification method is applied to detect transients, and the YAFTA algorithm is used to extract the magnetic features. Using 10 yr of data, we detect in total 7,483,827 blinkers, 2,082,162 ECBPs, and 1,188,839 XCBPs, respectively, with their birth rate of about 1.1 × 10−18 m−2 s−1, 3.8 × 10−19 m−2 s−1, and 1.5 × 10−19 m−2 s−1. We find that about 80% of blinkers are observed at the boundaries of supergranules, and 57% (34%) are associated with ECBPs (XCBPs). We further find that about 61%–80% of transients are associated with the isolated magnetic poles in the quiet Sun and that the normalized maximum intensities of the transients are correlated with the photospheric magnetic flux of poles via a power law. These results conspicuously show that these transients have a magnetic origin and their synchronized behavior provides further clues toward the understanding of the coupling among the different layers of the solar atmosphere. Our study further reveals that the appearance of these transients is strongly anticorrelated with the sunspots’ cycle. This finding can be relevant for a better understanding of solar dynamo and magnetic structures at different scales during the solar cycle.