bluuebunny/crossref_metadata_2025_split huggingface dataset:
INTERPRETASI JENIS BATUAN MENGGUNAKAN METODE GEOMAGNETIK PADA DAERAH TERAKUMULASINYA AIR TANAH DI BENA AMANUBAN SELATAN
Authors: Takaeb Yohanes , Sutaji Hadi Imam , Bernandus Bernandus 
Published: August 2019

Abstrak
Telah dilakukan penelitian interpretasi jenis batuan menggunakan metode geomagnetik pada daerah terakumulasinya air tanah di Bena Amanuban Selatan. Tujuan penelitian ini untuk menentukan pemetaan anomali magnetik bawah permukaan dan pola penyebaran batuan di sekitar daerah terakumulasinya air tanah. Akuisisi data menggunakan Proton Precession Magnetometer (PPM) tipe GSM–19T. Hasil pengukuran data lapangan berupa nilai medan magnet total dan variasi harian yang diolah serta diinterpretasikan secara kualitatif dan kuantitatif. Interpretasi kualitatif menunjukkan tiga pola anomali, yaitu anomali tinggi, sedang dan rendah. Anomali tinggi (sekitar 105 nT sampai 140 nT) pada bagian selatan dan barat daya diduga berupa batuan lempung dan batugamping. Anomali sedang (sekitar 70 nT sampai <105 nT) yang mendominasi lokasi penelitian diduga batuan lempung dan batu pasir. Anomali rendah (sekitar 40 nT sampai <70 nT) di bagian timur diduga batu gamping dan batu pasir. Interpretasi kuantitatif menunjukan struktur batuan yang diduga akuifer yaitu batu pasir memiliki suseptibilitas 6.7 x 10-5 – 3.56 x10-4 pada kedalaman 22.8 m serta batugamping yang bersifat meluluskan air dengan suseptibilitas 5.792 x 10-3 – 9.247 x 10-3 dengan kedalaman 75 m. Selain kedua batuan tersebut, terdapat batuan lempung dengan suseptibilitas 7.28 x 10-4 – 1.063 x 10-3 di kedalaman 13.8 m.
Kata kunci: Metode geomagnetik, suseptibilitas, akuifer.
Abstract
An interpretation of rock types has been done using geomagnetic method in the area of ​​accumulated groundwater in Bena Amanuban Selatan. The purpose of this study was to determine the mapping of subsurface magnetic anomalies and the pattern of rock distribution around the accumulated groundwater area. Data acquisition using Proton Precession Magnetometer (PPM) type GSM-19T. The results of field data measurements in the form of total magnetic field value and daily variations are processed and interpreted qualitatively and quantitatively. Qualitative interpretation shows three patterns of anomalies, namely high anomalies, moderate and low. High anomalies (about 105 nT to 140 nT) in the south and southwest are thought to be clay and limestone. Moderate anomalies (about 70 nT to <105 nT) that dominate the study sites are suspected clay and sandstone. Low anomalies (about 40 nT to <70 nT) in the eastern part are suspected of limestone and sandstone. Quantitative interpretation shows the suspected aquifer rock structure of sandstone has a susceptibility of 6.7 x 10-5 – 3.56 x10-4 at a depth of 22.8 m as well as a water-grinding limestone with the susceptibility of 5.792 x 10-3 – 9.247 x 10-3 with a depth of 75 m. In addition to these two rocks, there are clay rocks with the susceptibility of 7.28 x 10-4 – 1.063 x 10-3 at depth of 13.8 m.
Keywords: Geomagnetic method, susceptibility, aquifer.
ПолитическаяидентичностьСиро-Христианскогосоциума подвластью хулагуидских Ильханов(XIIIXIVвв.):некоторыенаблюдения
Authors: Koraev T.K. 
Published: August 2019

The article deals with a dramatically turbulent period in the history of Syriac Christianity, encompassing the late 13th and the early 14th centuries that coincided with the establishment, strengthening and collapse of the Mongol rule in Iran and Mesopotamia. The primary focus is on the two Syria communities the Western (Jacobite) and the Eastern (Assyrian) ones inhabiting the territories of modern North Iraq and South Turkey that were at the time one of the hotbeds of Christianity and homeland to numerous Arameic dialects. Unlike its neighbours, even though similar to them from the cultural an religious perspectives (especially the Armenians), the Syriac society showed an almost total absence of any clearcut traditional elite (to say nothing of aristocracy) that could have assumed administrative functions. Under these circumstances the Mongol invasion and the triumph of the Chinggisid rule in the Tigris Euphrates valley contributed to the formation, in the Eastern Syriac milieu, of a quasimonarchical form of administration that of the local princesgovernors (sing. malik, pl. muluk). For centuries to come the status of Malik passed through a long transformation in order to evolve from a bureaucratic figurehead (even notwithstanding the implied monarchial attributes) into a defacto local ruler of a highland community. The process of formation of the Malik rule and the peculiarities of Christian Malik rule in Mesopotamia is analysed through relevant data of the Syriac, Arab and Persian chroniclesСтатья посвящена драматически турбулентному периоду в история сирийского христианства, охватывающая конец 13го и начало 14 века, что совпало с установлением, усилением и крахом монгольского владычества в Иране и Месопотамия. Основное внимание уделяется двум сирийским общинам Западной (Якобитская) и Восточной (Ассирийская) населяющие территорию современного Северного Ирака и юга Турция, которая была в то время одним из очагов христианства и родиной многочисленных арамейских диалектов. В отличие от своих соседей, хотя подобно им с культурной и религиозной точек зрения (особенно армяне), сирийское общество показало почти полное отсутствие какихлибо четких традиционных элит (не говоря уже об аристократии), которые могли бы взять на себя административные функции. В этих условиях монгольское нашествие и триумф правления Чингизидов в долине ТиграЕвфрата способствовало формированию в Восточносирийской среде квазимонархической формы правления, администрация формировалась из местных князейнаместников (единсвт. Малик, множеств. Мулук). На протяжении веков статус Малика проходил через длительную трансформацию чтобы эволюционировать от бюрократического номинального руководителя (даже несмотря на подразумеваемые монархические атрибуты) в дефакто местного правителя. Процесс формирования правила Малика и особенности правление христианина Малика в Месопотамии анализируется с помощью соответствующих данных, взятых из сирийских, арабских и персидских хроник.
Битвазапрошлое:храмсвятогоГеоргия вИзраавэпицентре церковно-политическойборьбыконцаXIXв.
Authors: Kopot` E.M. 
Published: August 2019

The article brings up an obscure episode in the rivalry of the Orthodox and Melkite communities in Syria in the late 19th century. In order to strengthen their superiority over the Orthodox, the Uniates attempted to seize the church of St. George in Izraa, one of the oldest Christian temples in the region. To the Orthodox community it presented a threat coming from a wealthier enemy backed up by the See of Rome and the French embassy. The only ally the Antioch Patriarchate could lean on for support in the fight for its identity was the Russian Empire, a traditional protector of the Orthodox Arabs in the Middle East. The documents from the Foreign Affairs Archive of the Russian Empire, introduced to the scientific usage for the first time, present a unique opportunity to delve into the history of this conflict involving the higher officials of the Ottoman Empire as well as the Russian embassy in ConstantinopleВ статье рассматривается малоизвестный эпизод соперничества православной и Мелкитской общин в Сирии в конце XIX века. Чтобы укрепить свое превосходство над православными, униаты предприняли попытку захватить церковь Святого Георгия в Израа, один из старейших христианских храмов в регионе. Для православной общины он представлял угрозу, исходящую от более богатого врага, поддерживаемого Римским престолом и французским посольством. Единственным союзником, на которого Антиохийский патриархат мог опереться в борьбе за свою идентичность, была Российская Империя, традиционный защитник православных арабов на Ближнем Востоке. Документы из архива иностранных дел Российской Империи, введены в научный оборот впервые, уникальная возможность углубиться в историю этого конфликта с участием высших должностных лиц в Османской империи, а также российского посольства в Константинополе.
Psychological Conflict Between Men and Women in Susan Glaspell’s Trifles
Authors: Guswanto Doni , Husna Lailatul 
Published: August 2019

The problem in this paper is psychological conflict between men and women. In the Trifles drama by Susan Glaspell, women seem to have no freedom in terms of expressing opinions, ideas and ideas only because of male domination. Plus women feel inferior just because the man is superior. This is manifested in the act of having to obey what men say to women both in the family environment and in the community.
In this writing, the writer uses descriptive research as the method of collecting the data. As for the data analysis method, after determining the theory obtained from the related book, the formulation of the problem is analyzed using the theory of psychology. By using the theory of Sigmund Freud, the characters in the drama are then further analyzed to understand the shape, causes and consequences of a conflict. Authors carry out structural methods with understanding drama, male and female characters. Data collection techniques use qualitative techniques by taking notes in collecting primary data. In data analysis techniques, the author uses techniques by interpreting data.
The results of the research in this survey are: 1) Forms of conflict obtained from female leaders whose actions are limited by men. 2) The causes of conflict comes from movements of female figures who do not want to be underestimated by male figures. 3) As a result of the conflict, Mrs. Wright killed her husband because he could not stand the treatment of her husband anymore. In closing, this drama tells the story of conflict between men and women. The mutual respect is very important between men and women.
General Retaliation Against The Roman Empire as Seen in William Shakespeare’s Coriolanus
Authors: Hendria Ricky , Franchisca Sherly 
Published: August 2019

This reseacrh is titled "General Retaliation Against The Roman Empire As Seen In William Shakespeare's Coriolanus. In this research the author will discuss several issues, namely (1) How is Coriolanus's struggle in defending Rome's empire from enemy attacks? (2) What did Coriolanus do to avenge himself at the Roman empire? (3) What is the story of Coriolanus at the end of the story? the objectives of this research are (1) To analyze Coriolanus' life at the beginning of the story (2) To explain the cause of coriolanus to avenge his Roman empire (3) To study and explain how much Coriolanus's grudge to Rome to the tragic story he experienced.
The theory used in this research is literary psychology theory according to Sigmund Freud. This research uses a qualitative method. The object of research is the drama Coriolanus by William Shakespeare. Data sources are divided into two, namely primary data sources and secondary data sources. The primary data source is the drama script itself. Secondary data sources are text texts and several references related to research. The data collection technique is taking notes. The technical analysis of the data is descriptive analysis.
The results of the study show the following conclusions. First, the responsibility of a general in maintaining the sovereignty of his kingdom. Second, feelings of resentment arise when a struggle is not properly appreciated. Third, someone's revenge towards others can have fatal consequences and can even end in a tragic death.
Topofobia: a representação dos espaços opressivos em “Amada” de Toni Morrison
Authors: Vieira Wellington Neves , Seidel Roberto Henrique 
Published: August 2019

O objetivo desta pesquisa é identificar as representações dos espaços opressivos na obra Amada de Toni Morrison, a partir de uma percepção sobre o espaço, demonstrando a relação dos espaços ocupados pelos personagens negros, na transmissão de sentimentos de topofobia. A metodologia empregada é de caráter teórico, qualitativo-descritivo. Na intenção de esquematizar a pesquisa literária por meio de análises explicativas, descritivas e exploratórias, adentra-se o campo da Geografia Humanista como base de sustentação do estudo. Discute-se a Geografia Humanista do ponto de vista espacial. Por fim, averígua-se a relação dos personagens com os espaços opressivos. Constatou-se ao final da pesquisa que as análises dos espaços que foram feitas no romance “Amada” transmitem a revitalização de um passado à procura de dar voz a uma nova realidade histórica, o que poderá ser compreendido como a constituição de um espaço para uma “alteridade” que desafia e resiste ao discurso dominante.
Nacionalismo e hibridismos identitários no romance histórico Mulheres de Cinzas, de Mia Couto
Authors: Moura Adriano Carlos 
Published: August 2019

Mulheres de Cinzas, primeiro livro da trilogia histórica Areias do Imperador de Mia Couto, é um romance narrado sob a perspectiva de uma jovem moçambicana e de um soldado português alternadamente. Trata-se de um romance histórico sobre o período em que o Sul de Moçambique era governado por Ngungunyane, último imperador do Estado de Gaza que, no final do século XIX, ameaçava o domínio colonial. Este artigo é resultado de um estudo da obra, com a finalidade de investigar o papel da língua como construção da identidade individual e coletiva numa sociedade em conflito entre colonizados e colonizadores, e a hibridez entre ambos como marca da experiência colonial. Parte-se, inicialmente, dos estudos históricos de Erick Hobsbawm sobre nação, língua e nacionalismo, a partir de 1780, para compreender como a maioria dos países ocidentais construiu esses conceitos. Em seguida, o romance é analisado como narrativa performativa sobre a nação, considerando seu contexto de produção (Moçambique pós-colonial), entendendo o termo “performativo” na acepção concebida por Homi Bhabha e suas reflexões sobre identidade. Nesse contexto, a língua é percebida não como um elemento de comunicação apenas, mas também de conflito no espaço lusófono.
Compact Disks in a High-resolution ALMA Survey of Dust Structures in the Taurus Molecular Cloud
Authors: Long 龙 Feng 凤 , Herczeg 沈 Gregory J. 雷歌 , Harsono Daniel , Pinilla Paola , Tazzari Marco , Manara Carlo F. , Pascucci Ilaria , Cabrit Sylvie , Nisini Brunella , Johnstone Doug , Edwards Suzan , Salyk Colette , Menard Francois , Lodato Giuseppe , Boehler Yann , Mace Gregory N. , Liu Yao , Mulders Gijs D. , Hendler Nathanial , Ragusa Enrico , Fischer William J. , Banzatti Andrea , Rigliaco Elisabetta , van de Plas Gerrit , Dipierro Giovanni , Gully-Santiago Michael , Lopez-Valdivia Ricardo 
Published: August 2019

Abstract
We present a high-resolution (∼0.″12, ∼16 au, mean sensitivity of 50 μJy beam−1 at 225 GHz) snapshot survey of 32 protoplanetary disks around young stars with spectral type earlier than M3 in the Taurus star-forming region using the Atacama Large Millimeter Array. This sample includes most mid-infrared excess members that were not previously imaged at high spatial resolution, excluding close binaries and objects with high extinction, thereby providing a more representative look at disk properties at 1–2 Myr. Our 1.3 mm continuum maps reveal 12 disks with prominent dust gaps and rings, 2 of which are around primary stars in wide binaries, and 20 disks with no resolved features at the observed resolution (hereafter smooth disks), 8 of which are around the primary star in wide binaries. The smooth disks were classified based on their lack of resolved substructures, but their most prominent property is that they are all compact with small effective emission radii (R
eff,95% ≲ 50 au). In contrast, all disks with R
eff,95% of at least 55 au in our sample show detectable substructures. Nevertheless, their inner emission cores (inside the resolved gaps) have similar peak brightness, power-law profiles, and transition radii to the compact smooth disks, so the primary difference between these two categories is the lack of outer substructures in the latter. These compact disks may lose their outer disk through fast radial drift without dust trapping, or they might be born with small sizes. The compact dust disks, as well as the inner disk cores of extended ring disks, that look smooth at the current resolution will likely show small-scale or low-contrast substructures at higher resolution. The correlation between disk size and disk luminosity correlation demonstrates that some of the compact disks are optically thick at millimeter wavelengths.
The Radial Acceleration Relation Is a Natural Consequence of the Baryonic Tully–Fisher Relation
Authors: Wheeler Coral , Hopkins Philip F. , Doré Olivier 
Published: August 2019

Abstract
Galaxies covering several orders of magnitude in stellar mass and a variety of Hubble types have been shown to follow the radial acceleration relation (RAR), a relationship between

, the observed circular acceleration of the galaxy, and

, the acceleration due to the total baryonic mass of the galaxy. For accelerations above

,

traces

, asymptoting to the 1:1 line. Below this scale, there is a break in the relation such that

. We show that the RAR slope, scatter, and the acceleration scale are all natural consequences of the well-known baryonic Tully–Fisher relation (BTFR). We further demonstrate that galaxies with a variety of baryonic and dark matter (DM) profiles and a wide range of dark halo and galaxy properties (well beyond those expected in Cold Dark Matter (CDM) theory) lie on the RAR if we simply require that their rotation curves satisfy the BTFR. We explore conditions needed to break this degeneracy: subkiloparsec resolved rotation curves inside of cored DM-dominated profiles and/or outside

could lie on BTFR but deviate in the RAR, providing new constraints on DM.
The CARMA-NRO Orion Survey: Core Emergence and Kinematics in the Orion A Cloud
Authors: Kong Shuo , Arce Héctor G. , Sargent Anneila I. , Mairs Steve , Klessen Ralf S. , Bally John , Padoan Paolo , Smith Rowan J. , Maureira María José , Carpenter John M. , Ginsburg Adam , Stutz Amelia M. , Goldsmith Paul , Meingast Stefan , McGehee Peregrine , Sánchez-Monge Álvaro , Suri Sümeyye , Pineda Jaime E. , Alves João , Feddersen Jesse R. , Kauffmann Jens , Schilke Peter 
Published: August 2019

Abstract
We have investigated the formation and kinematics of submillimeter (submm) continuum cores in the Orion A molecular cloud. A comparison between submm continuum and near-infrared extinction shows a continuum core detection threshold of A

V
∼ 5–10 mag. The threshold is similar to the star formation extinction threshold of A

V
∼ 7 mag proposed by recent work, suggesting a universal star formation extinction threshold among clouds within 500 pc to the Sun. A comparison between the Orion A cloud and a massive infrared dark cloud G28.37+0.07 indicates that Orion A produces more dense gas within the extinction range 15 mag ≲ A

V
≲ 60 mag. Using data from the CARMA-NRO Orion Survey, we find that dense cores in the integral-shaped filament (ISF) show subsonic core-to-envelope velocity dispersion that is significantly less than the local envelope line dispersion, similar to what has been found in nearby clouds. Dynamical analysis indicates that the cores are bound to the ISF. An oscillatory core-to-envelope motion is detected along the ISF. Its origin is to be further explored.
UVIT Open Cluster Study. I. Detection of a White Dwarf Companion to a Blue Straggler in M67: Evidence of Formation through Mass Transfer
Authors: Sindhu N. , Subramaniam Annapurni , Jadhav Vikrant V. , Chatterjee Sourav , Geller Aaron M. , Knigge Christian , Leigh Nathan , Puzia Thomas H. , Shara Michael , Simunovic Mirko 
Published: August 2019

Abstract
The old open cluster M67, populated with blue straggler stars (BSSs), is a well-known test bed to study the BSS formation pathways. Here, we report the first direct detection of a white dwarf (WD) companion to a BSS in M67, using far-UV images from the Ultra-Violet Imaging telescope on ASTROSAT. Near-simultaneous observations in three far-UV bands combined with Galaxy Evolution Explorer, International Ultraviolet Explorer, and ground- and space-based photometric data covering a 0.14–11.5 μm range for WOCS1007 were found to require a binary fit to its spectral energy distribution (SED), consisting of a BSS and a hot companion. On the other hand, a single spectral fit was found to be satisfactory for the SEDs of two other BSSs, WOCS1006 and WOCS2011, with the latter showing a deficient far-UV flux. The hot companion of WOCS1007 is found to have a

∼ 13,250–13,750 K and a radius of 0.09 ± 0.01

. A comparison with WD models suggests it to be a low-mass WD (∼

), in agreement with the kinematic mass from the literature. As a low-mass WD (<

) necessitates formation through mass transfer in close binaries, WOCS1007 with a known period of 4.2 days along with its fast rotation, is likely to be formed by a case A or case B binary evolution.
Active Galactic Nucleus Pairs from the Sloan Digital Sky Survey. III. Chandra X-Ray Observations Unveil Obscured Double Nuclei
Authors: Hou Meicun , Liu Xin , Guo Hengxiao , Li Zhiyuan , Shen Yue , Green Paul J. 
Published: August 2019

Abstract
We present Chandra ACIS-S X-ray imaging spectroscopy for five dual active galactic nucleus (AGN) candidates. Our targets were drawn from a sample of 1286 [O III]-selected AGN pairs systematically selected from the Sloan Digital Sky Survey Seventh Data Release. Each of the targets contains two nuclei separated by ∼3–9 kpc in projection, both of which are optically classified as Type 2 (obscured) AGNs based on diagnostic ratios of the narrow emission lines. Combined with independent, empirical star formation rate estimates based on the host-galaxy stellar continua, the new Chandra X-ray observations allow us to evaluate the dual-AGN hypothesis for each merging system. We confirm two (SDSS J0907+5203 and SDSS J1544+0446) of the five targets as bona fide dual AGNs. For the other three targets, the existing data are consistent with the dual-AGN scenario, but we cannot rule out the possibility of stellar/shock heating and/or one AGN ionizing both gaseous components in the merger. The average X-ray-to-[O III] luminosity ratio in our targets seems to be systematically smaller than that observed in single AGNs but is higher than that seen in dual AGNs selected from AGNs with double-peaked narrow emission lines. We suggest that the systematically smaller X-ray-to-[O III] luminosity ratio observed in dual AGNs than in single AGNs is due to a high nuclear gas column likely from strong merger-induced inflows. Unlike double-peaked-[O III]-selected dual AGNs, the new sample selected from resolved galaxy pairs are not subject to the orientation bias caused by the double-peak line-of-sight velocity splitting selection, which also contributes to lowering the X-ray-to-[O III] luminosity ratio.
Biodiversity of Early Holocene large mammals from the territory of Bulgaria according to remains from archaeological sites
Authors: Karastoyanova Nadezhda 
Published: August 2019

Animal remains from archeological sites give a rather good sample of data, showing habitats and biodiversity during the early Holocene . In multiple settlements in the Eastern Balkans, there are numerous remains of wild mammals that were hunted by humans through the prehistory (7200-5800 BP). This gives a general idea of the habitats around and near the settlements. Such deposits of animal remains are the main source of data on fauna during this period and give us information on the processes leading to the extinction of some species.
This paper analyzes more than 26000 animal remains (bones, horns, antlers and teeth) from large mammals from orders: Аrtiodactyla, Perissodactyla and Carnivora from 4 still unpublished deposits from Bulgaria. I summarize data from already published remains from 33 sites in East Balkans. These analyses provide a general picture of both habitats and biodiversity and some of the major factors that caused extinction of some large mammals in Bulgaria during the early Holocene.