bluuebunny/crossref_metadata_2025_split huggingface dataset:
Ruptured Right Cornual Pregnancy
Authors: Pokhrel Shreesiya , Dangal Ganesh , Karki Aruna , Pradhan Hema Kumari , Shrestha Ranjana , Bhattachan Kabin , Thapa Shekhar , Paudel Rekha , Bajracharya Nishma 
Published: November 2018

The ectopic implantation is implantation of fertilized ovum outside the uterine cavity, ampulla of fallopian tube being the most common site. A cornual or interstitial pregnancy is an ectopic pregnancy that develops in the interstitial portion of the fallopian tube which is one of the most hazardous type of ectopic gestation. Treatment depends on the week of gestation at the time of diagnosis, level of serum β HCG, findings of ultrasonography, hemodynamic stability of the patient and the choice of future fertility. In this case report, we present a case which was previously misdiagnosed as a case of missed abortion at 8 weeks of gestation by transabdominal ultrasound and patient underwent medical abortion with mefipristione and misoprostolandafter 1 month presented with pain abdomen and was confirmed as extrauterine pregnancy by transabdominal ultrasound followed by surgical management.
Use of Three-Dimensional Printing Models for Veterinary Medical Education: Impact on Learning How to Identify Canine Vertebral Fractures
Authors: Suñol Anna , Aige Vicente , Morales Carles , López-Beltran Marta , Feliu-Pascual Alejandro Luján , Puig Jordi 
Published: November 2018

Vertebral fractures and luxations are common causes of neurological emergencies in small-animal patients. The objective of this study was to evaluate the impact of three-dimensional printing (3Dp) models on how veterinary students understand and learn to identify canine spinal fractures and to compare 3Dp models to computed tomography (CT) images and three-dimensional CT (3D-CT) reconstructions. Three spinal fracture models were generated by 3Dp. Sixty first-year veterinary students were randomized into three teaching module groups (CT, 3D-CT, or 3Dp) and asked to answer a multiple-choice questionnaire with 12 questions that covered normal spinal anatomy and the identification of vertebral fractures. We used four additional questions to evaluate the overall learning experience and knowledge acquisition. Results showed that students in the 3Dp group performed significantly better than those in the CT ( p < .001) and the 3D-CT ( p < .001) groups. Students in the 3Dp and 3D-CT groups answered all questions more quickly than the CT group (3Dp versus CT, p < .001; 3D-CTversus CT, p < .001), with no significant differences between the 3Dp and 3D-CT groups ( p = .051). Only the degree of knowledge acquisition that the students considered they had acquired during the session showed significant differences between groups ( p = .01). In conclusion, across first-year veterinary students, 3Dp models facilitated learning about normal canine vertebral anatomy and markedly improved the identification of canine spinal fractures. Three-dimensional printing models are an easy and inexpensive teaching method that could be incorporated into veterinary neuroanatomy classes to improve learning in undergraduate students.
ANALISA KUALITAS PELAYANAN MENPENGARUHI KEPUASAN PASIEN BPJS (BADAN PENYELENGGARA JAMINAN SOSIAL) PADA RUMAH SAKIT STROKE NASIONAL BUKITTINGGI
Authors: Syaleh Hariman 
Published: November 2018

Penelitian ini bertujuan untuk menjelaskan apakah kualitas pelayanan mempengaruhi kepuasan pasien BPJS yang di tinjau dari dimensi bukti fisik, kehandalan, daya tanggap, jaminan dan empati. Sampel dalam penelitian ini terdiri dari 100 orang responden dan data diperoleh dengan menyebarkan kuesioner kepada pasien rawat inap yang berada di Rumah Sakit Stroke Nasional Bukittinggi dan di analisis dengan metode analisa regresi linear berganda, uji T,Uji F serta Uji Koefesien Detarmine (R2) dengan bantuan Software SPSS 21 for Windows. Hasil penelitian menunjukan bahwa ke 5 variabel yaitu : variabel bukti fisik memiliki pengaruh yang positif dan signifikan terhadap kepuasan pasien, begitu juga dengan variabel kedua kehandalan memiliki pengaruh yang positif dan signifikan terhadap kepuasan pasien dan yang ketiga variabel daya tanggap memiliki pengaruh yang positif dan signifikan terhadap kepuasan pasien yang keempat jaminan memiliki pengaruh yang positif dan signifikan terhadap kepuasan pasien dan empati memiliki pengaruh yang positif dan signifikan terhadap kepuasan pasien rawat inap BPJS pada Rumah Sakit Stroke Nasional Bukittinggi. Penulis mendapatkan kesimpulan dari kelima variabel yang penulis teliti baik secara parsial maupun simultan memiliki pengaruh positif signifikan terhadap kepuasan pasien BPJS pada Rumah Sakit Stroke Nasional Bukittinggi.
Kata kunci : kualitas pelayanan; kepuasan.
Phisical Function (Motor Activity) Pada Pasien Kritis Dengan Sedation Di Intensive Care Unit
Authors: Suwardianto Heru , Prasetyo Awal , Utami Reni Sulung 
Published: November 2018

Introduction: Critical patients are patients who potentially get reversible dysfunction in one or more life-threatening organs and require they require care in the Intensive Care Unit (ICU). Method: The objective of this research is to analyze the physical function-tardive dyskinesia on critical patients with sedation in ICU. The design of this research is crossectional. The population is all critical patients in ICU Baptist Hospital Kediri. The sample is 41 respondents based on the inclusion and exclusion criteria in the total sampling. The independent variable is giving the sedation and the dependent variable is physical function-tardive dyskinesia. The data was collected using observation sheets. Result: The result shows that giving a sedation can decrease the physical function in the form of motor activity; response of noxious stimuli (7.3%), response to touch or calling name (19,5%) and the incresing score of agitation and co-operative (4.9%). Symptoms of tardive dyskinesia increased after sedation in the form of tongue prostrusion (4.9%), lip smacking puckering and pursing (2.4%), and rapid movements of the arms and legs. Administration of sedation in the first 24-hour ICU patient affects the physical function of the critical patients (p = 0.005). Conclusion: Giving sedation affects the change of patiens’ physical funcion. Therefore, prevention on the effects of sedation and treatment during ICU is needed in order to avoid a decrease in the physical function of critical patients. Keyword: physical function, tardive dyskinesia, sedation, critical patient, ICU
Dragon Ball Popularity in Spain Compared to Current Delocalized Models of Consumption
Authors: Santiago Iglesia José Andrés 
Published: November 2018

The development of anime and manga in Spain in the late 70s and 80s and their boom in the early 90s mimics its progression in the two prominent European markets, Italy and France. Most of the mainstream anime series broadcasted in Spain were originally imported from Italian media conglomerate Fininvest as well as French licensing companies.

In February of 1990, Dragon Ball, a TV adaptation of the manga created by the renowned cartoonist Toriyama Akira, premiered in Spain. However, Dragon Ball was not an immediate phenomenon. The ‘when,’ ‘where’ and ‘how’ differ from any other broadly popular anime/manga series in Spain or any other major European market, due to the specificity of the Spanish «Autonomous Communities’» cultural, political and administrative division. Dragon Ball first premiered in Spain via several regional broadcasters — TVG, TV3 and ETB (Galicia, Catalonia and Basque Country) — with only a few weeks in between, dubbed not in Castilian Spanish but in the respective co-official languages (Galician, Catalonian, Basque), growing into an independent social phenomenon within these regions before it spread nationwide years later.
Thanks to Dragon Ball, anime as a cultural platform in Spain influenced many people by expanding fandom boundaries to a broader social spectrum, turning anime and manga into mainstream mediums and – while both publishers and merchandising companies failed to anticipate such a significant social impact – setting the foundations of the Spanish manga/anime industry. It is clear that no other anime series has ever triggered such a cultural phenomenon, in terms of general success, social dissemination and broadcast mechanics. Therefore, in this article I will try to examine Dragon Ball in Spain as a complex model, and analyse its unique model of intermedia growth
Post-Traumatic Stress Syndrome (PTSS) in Nurses Post-Earthquake Disaster in Indonesia
Authors: (Corresponding author) Mustikasari , Sahar Junaiti , Fadhillah Harif , Pratiwi Anggi 
Published: November 2018

Post-traumatic stress syndrome (PTSS) may be experienced by individuals who were traumatized by unpleasant experiences, such as earthquakes, which occur suddenly, and are diffi cult to predict. This study is aimed to explore PTSS experienced by nurse survivor following earthquakes in several areas in Indonesia. A qualitative study was conducted to participants with the following criteria: nurses who were actively working in the primary level health care services (health centers) and had experienced PTSS as determined by screening results. The study was conducted in regencies/cities that have experienced earthquakes in West Sumatra, North Sulawesi, Yogyakarta, East Java, and Banten. Data were collected for 3 months, between September and November 2011. Participants were recruited
through purposive sampling according to the inclusion criteria for PTSS screening (experienced 2-3 years of grief). Ten participants agreed to be interviewed. Data were analyzed by thematic analysis. Two main themes emerged consisting of physical and psychological responses of nurses. Trembling and being scared have been the consistent response up to several years after the incident. The results of the study can serve as source of information for developing nursing skills in the prevention and mitigation stage of disaster, as well as for the formulation of supportive policies.
Effect of Nurse Performance in Patient Safety Target Based on Knowledge Management: SECI on Quality of Nursing Services
Authors: (Corresponding author) Harif Fadhillah , - Nursalam , Hadi Muhammad 
Published: November 2018

Appropriate knowledge management will improve nurse performance. There have been numerous studies on nurse performance, but studies on nurse performance of Knowledge management: SECI in Indonesia have not been widely reported and therefore researchers interested in conducting this study. This study aims at identifying the effect of performance in patient safety target based on Knowledge Management: SECI on the quality of nursing services in Jakarta Islamic Hospital of Pondok Kopi. The study employed quasi experimental design of pre and posttest with control group. The respondents were nurses who worked in the inpatient unit with a sample size of 24 respondents in the intervention group and 37 respondents in the control group. The instrument used to measure pre-posttest was patient safety developed by Nasution (2013) with validity value of 0.444-0.772 and reliability of Cronbach’s Alpha of 0.950; and the adverse events developed by the researchers. Intervention
protocols in the form of performance in patient safety target based on Knowledge Management: SECI were given through training. The analysis employed statistical tests of Mann Whitney and Wilcoxon. The study found that there was a change in patient safety before and after intervention in the intervention group rather than in the control group. There were differences in the scores of patient safety/quality of nursing care after treatment in the intervention group and the control group. The study recommends regular training for nurses concerning performance in patient safety target based on Knowledge Management: SECI, and further studies in different hospitals.
BURSA ESKİ KAPLICA: MİMAR VE YAPININ ORİJİNİ MESELESİ
Authors: YILMAZYAŞAR Hasan 
Published: November 2018

Bursa Eski Kaplıca’nın kesin inşa tarihini ortaya koyan her hangi bir belge bulunmamakla birlikte gerek Osmanlı kronikleri, gerekse arşiv belgelerinde yer alan bilgiler yapının I. Murad döneminde inşa edilmiş olduğunu ortaya koyar. Bursa Eski Kaplıca’nın “Yıldızvari Sıcaklıklı Tip” olarak tanımlanan ve antik dönem hamamları ile ilişkilendirilen sekizgen planlı sıcaklık bölümünün dört köşesinde yer alan yarım daire nişlerden ibaret mekan düzeninin öncül örnekleri Roma ve Geç Antik dönem Hamamlarında karşımıza çıkmaktadır. Bu plan şeması Roma Mauseliumları ile 6. yüzyıl Bizans vaftizhaneleri ve bazı kiliselerde de tercih edilmiştir. Söz konusu plan tipi ile yapının cephe düzeni ve malzeme teknik detaylarında karşımıza çıkan Geç Dönem Bizans Mimarisi’nde yaygın kullanımı gözlenen bazı unsurlar, Bursa Eski Kaplıca’nın özellikle yapıyı gören Avrupalı seyyahlar tarafından bir Bizans yapısı olarak tanıtılmasına sebep olmuş, bazı araştırmacılar seyyahlarla aynı görüşü savunmuş; bazı araştırmacılar ise kaplıcanın Türk mimar ve ustalar tarafından inşa edildiği yönünde görüş bildirmişlerdir. Çok sayıda yayında değinilen bir yapı olmasına karşın Eski Kaplıca monografik bir çalışmaya konu olmamış, yapıya dair belge ve bilgiler kapsamlı bir değerlendirmede ele alınmamıştır. Yapının mimarı ve orijini hususunda ise farklı görüşler güncelliğini korumakta, bir fikir birliğine varılmadığı anlaşılmaktadır. Bu makalede yapının tarihlendirilmesine dair yeni bazı tespitler ile birlikte, esas olarak yapının orijini ve mimarı konusu ele alınarak değerlendirilecektir.
Corrosion des coupoles de plafond par les fluctuations de pression de l'air emprisonné
Authors: Lismonde Baudouin 
Published: November 2018

Nous proposons un nouveau mécanisme de creusement des réseaux semi-noyés et nous l'appliquons plus particulièrement à la formation des coupoles de plafond. Nous supposons que certaines coupoles prennent naissance dans la zone épinoyée des grottes. Les fluctuations du niveau piézomé-trique de l'eau emprisonnent un volume d'air et le mettent en pression. La pression partielle du gaz carbonique augmente en proportion. Cette compression est quasi isotherme et un brouillard se forme dans l'air. Les gouttes de ce brouillard récupèrent le gaz carbonique et le ramènent sur les parois et l'eau. D'où une reprise de corrosion. Par exemple une mise en charge de 10 m d'une bulle d'air à PCO2 = 3.10-3 conduit à une dissolution supplémentaire atteignant 1 g/kg d'air.
Nous présentons un modèle numérique simplifié de formation de coupole.
Internal Structures of Molecular Clouds in the LMC Revealed by ALMA
Authors: Sawada Tsuyoshi , Koda Jin , Hasegawa Tetsuo 
Published: November 2018

Abstract
We observed five giant molecular clouds (GMCs) in the Large Magellanic Cloud (LMC) in the 12CO J = 1–0 line using the Atacama Large Millimeter/submillimeter Array (ALMA). The sample includes four GMCs with some signs of star formation—either YSOs, H ii regions, and/or young clusters—and one quiescent GMC without any sign of massive star formation. The data from the ALMA 12 m, 7 m, and Total-Power arrays are jointly deconvolved to obtain high-fidelity images at high spatial resolution (3″ = 0.7 pc). The four star-forming GMCs show very complex structures with clumps and filaments. The quiescent GMC shows a relatively diffuse, extended emission distribution without prominent clumps or filaments. This difference is similar to that between structured molecular gas in Milky Way spiral arms and unstructured gas in the inter-arm regions. We characterize the difference with the brightness distribution function and brightness distribution index. In conjunction with other ALMA studies of GMCs in the LMC, the five GMCs tentatively form an evolutionary trend: from less structured, quiescent GMCs to more structured, actively star-forming GMCs. A future ALMA study will be able to map molecular clouds over the LMC and reveal the evolutionary sequence of molecular clouds.
Spatial Expansion and Speeds of Type III Electron Beam Sources in the Solar Corona
Authors: Reid Hamish A. S. , Kontar Eduard P. 
Published: November 2018

Abstract
A component of space weather, electron beams are routinely accelerated in the solar atmosphere and propagate through interplanetary space. Electron beams interact with Langmuir waves resulting in type III radio bursts. They expand along the trajectory and, using kinetic simulations, we explore the expansion as the electrons propagate away from the Sun. Specifically, we investigate the front, peak, and back of the electron beam in space from derived radio brightness temperatures of fundamental type III emission. The front of the electron beam travels at speeds from 0.2c to 0.7c, significantly faster than the back of the beam, which travels at speeds between 0.12c and 0.35c. The difference in speed between the front and the back elongates the electron beam in time. The rate of beam elongation has a 0.98 correlation coefficient with the peak velocity, in line with predictions from type III observations. The inferred speeds of electron beams initially increase close to the acceleration region and then decrease through the solar corona. Larger starting densities and harder initial spectral indices result in longer and faster type III sources. Faster electron beams have higher beam energy densities, and produce type IIIs with higher peak brightness temperatures and shorter FWHM durations. Higher background plasma temperatures also increase speed, particularly at the back of the beam. We show how our predictions of electron beam evolution influences type III bandwidth and drift rates. Our radial predictions of electron beam speed and expansion can be tested by the upcoming in situ electron beam measurements made by Solar Orbiter and Parker Solar Probe.
Distances and Kinematics of Gould Belt Star-forming Regions with Gaia DR2 Results
Authors: Dzib Sergio A. , Loinard Laurent , Ortiz-León Gisela N. , Rodríguez Luis F. , Galli Phillip A. B. 
Published: November 2018

Abstract
We present an analysis of the astrometric results from the Gaia second data release (DR2) for young stellar objects (YSOs) in star-forming regions related to the Gould Belt (GB). These regions are Barnard 59, Lupus 1 to 4, Chamaeleon I and II, ϵ Chamaeleontis, the Cepheus flare, IC 5146, and Corona Australis. The mean distance to the YSOs in each region is consistent with earlier estimations, though a significant improvement in the final errors was obtained. The mean distances to the star-forming regions were used to fit an ellipsoid of size (358 ± 7) ×(316 ± 13) × (70 ± 4) pc3, centered at (X
0, Y
0, Z
0) = (−82 ± 15, 39 ± 7, −25 ± 4) pc, consistent with recently determined parameters of the GB. The mean proper motions were combined with radial velocities from the literature to obtain the three-dimensional motions of the star-forming regions, which are consistent with a general expansion of the GB. We estimate that this expansion is occurring at a velocity of 2.5 ± 0.1 km s−1. This is the first time that motions of YSOs have been used to investigate the kinematics of the GB. As an interesting side result, we also identified stars with large peculiar velocities.
Spectroscopy of the Type Ic Supernova SN 2017iuk Associated with Low-redshift GRB 171205A
Authors: Wang J. , Zhu Z. P. , Xu D. , Xin L. P. , Deng J. S. , Qiu Y. L. , Qiu P. , Wang H. J. , Zhang J. B. , Wei J. Y. 
Published: November 2018

Abstract
We here report a spectroscopic monitor for the supernova (SN) SN 2017iuk associated with the long-duration low-luminosity gamma-ray burst (GRB) GRB 171205A at a redshift of 0.037, which is up to now the third GRB–SN event away from us. Our spectroscopic observations and spectral analysis allow us to identify SN 2017iuk as a typical broad-line Type Ic SN. A comparison study suggests that the Type IcBL SN 2017iuk resembles SN 2006aj in the following aspects: (1) similar spectra at the nearby epochs, (2) comparable evolution of the photospheric velocity obtained from the measurements based on both the Si ii
λ6355 line and spectral modeling, and (3) comparable explosion parameters. This analogy could imply the formation of a neutron star in the core collapse of GRB 171205A/SN 2017iuk as previously suggested in GRB 060218/SN 2006aj. The properties of the host galaxy are discussed, which suggest that GRB 171205A/SN 2017iuk occurred in an early-type (S0), high-mass, star-forming galaxy with low specific star formation rate and solar metallicity.
Comparing Chandra and Hubble in the Northern Disk of M31
Authors: Williams Benjamin F. , Lazzarini Margaret , Plucinsky Paul P. , Sasaki Manami , Antoniou Vallia , Vulic Neven , Eracleous Michael , Long Knox S. , Binder Breanna , Dalcanton Julianne J. , Lewis Alexia R. , Weisz Daniel R. 
Published: November 2018

Abstract
The X-ray source populations within galaxies are typically difficult to identify and classify with X-ray data alone. We are able to break through this barrier by combining deep new Chandra ACIS-I observations with extensive Hubble Space Telescope (HST) imaging from the Panchromatic Hubble Andromeda Treasury of the M31 disk. We detect 373 X-ray sources down to 0.35–8.0 keV flux of 10−15 erg cm−2 s−1 over 0.4 square degrees, 170 of which are reported for the first time. We identify optical counterpart candidates for 188 of the 373 sources, after using the HST data to correct the absolute astrometry of our Chandra imaging to 0.″1. While 58 of these 188 are associated with point sources potentially in M31, over half (107) of the counterpart candidates are extended background galaxies, 5 are star clusters, 12 are foreground stars, and 6 are supernova remnants. Sources with no clear counterpart candidate are most likely to be undetected background galaxies and low-mass X-ray binaries in M31. The hardest sources in the 1–8 keV band tend to be matched to background galaxies. The 58 point sources that are not consistent with foreground stars are bright enough that they could be high-mass stars in M31; however, all but 8 have optical colors inconsistent with single stars, suggesting that many could be background galaxies or binary counterparts. For point-like counterparts, we examine the star formation history of the surrounding stellar populations to look for a young component that could be associated with a high-mass X-ray binary. About one-third of the point sources are not physically associated with a young population, and are therefore more likely to be background galaxies. For the 40 point-like counterpart candidates associated with young populations, we find that their age distribution has two peaks at 15–20 Myr and 40–50 Myr. If we only consider the 8 counterpart candidates with typical high-mass main-sequence optical star colors, their age distribution peaks mimic those of the sample of 40. Finally, we find that intrinsic faintness, and not extinction, is the main limitation for finding further counterpart candidates.