bluuebunny/crossref_metadata_2025_split huggingface dataset:
CONTENTION PHYSIQUE PASSIVE
Authors: Oliveira Magnolia Ouriques de 
Published: June 2019

J'ai pu constater au sein de mon équipe, que la contention physique passive, est une proposition quasi systématique evoqué par l'equipe pour répondre aux problèmes de chutes causés par la perte d'autonomie. Mais non seulement en cas de chutes mais aussi en cas d'agressivité de ces personnes contre elles-mêmes ou envers les autres.Je pense que ce sont des propositions qui révèlent davantage d'un héritage de pratiques institutionnelles qu'une véritable réflexion sur la nécessité même de cet acte.Pierre Bourdieu sociologue Français dans ses études sur le concept d'Habitus dit: "L'habitus c’est le résultat d’un ensemble de pratiques qui s’est constitué au fil du temps, a été capitalisé et se transmet de génération en génération par la confrontation à la réalité".Dès l’antiquité la contrainte physique a été un recours au traitement de la guérison de personnes considérées comme folles, agitées. De nos jours, cette pratique est toujours requise lorsque l’équipe se sent incapable de maîtriser une situation.Ce travail d'observation a été réalisé au sein d'un Etablissement accueillant des personnes en situation d'handicap moteurs et intellectuel dont l’Age varie entre 45 ans à 70 ans.Dans cet écrit, je vais mettre en lumière ce constat en montrant les raisons de cette pratique de la contention physique passif, tout en donnant quelques pistes de réflexion pour atténuer ce problème car je pense qu'il y a nécessité de sensibiliser l'equipe a une nouvelle pratique.
PENGARUH TERAPI BEKAM DALAM MENURUNKAN TEKANAN DARAH PADA PASIEN HIPERTENSI DI RUMAH BEKAM PALEMBANG
Authors: Surahmat Raden , Damayanti Nanda Rizki 
Published: June 2019

Penyakit hipertensi menjadi salah satu masalah utama dalam kesehatan masyarakat Indonesia, terutama terjadi di negara berkembang. Upaya untuk mencegah terjadinya tekanan darah tinggi salah satunya dengan terapi bekam. Penelitian ini bertujuan untuk mengetahui pengaruh terapi bekam dalam menurunkan tekanan darah pada pasien hipertensi di Rumah Bekam Palembang Tahun 2016. Penelitian ini merupakan penelitian kuantitatif dengan metode one group pre test post test design dengan sampel berjumlah 75 orang Palembang pengambilan sampel menggunakan teknik Accidental Sampling. Pengumpulan data menggunakan kuesioner dan pengukuran tekanan darah. Analisis bivariat menggunakan uji wilcoxon (? = 0,05). Penelitian ini dilaksanakan pada tanggal 18 Januari - 13 Februari 2016 di Rumah Bekam Palembang. Hasil dari penelitian ini menunjukkan bahwa didapatkan klasifikasi tekanan darah sebelum terapi bekam dengan nilai mean 3,47 dan standar deviasi 0,502, klasifikasi tekanan darah setelah dilakukan terapi bekam dengan nilai mean 2,05 dan standar deviasi 0,853. Hasil uji bivariat dengan metode wilcoxon didapatkan nilai p value 0,000 (<0,05) menunjukkan ada pengaruh tekanan darah sebelum terapi bekam dengan tekanan darah setelah terapi bekam. Maka dapat disimpulkan ada perbedaan yang signifikan terapi bekam terhadap tekanan darah sebelum dan setelah dilakukan terapi bekam di Rumah Bekam Palembang Tahun 2016. Disarankan kepada pihak Rumah Bekam Palembang agar dapat terus menyelenggarakan pengobatan alternatif bekam serta meningkatkan promosi kepada masyarakat agar masyarakat makin mengetahui manfaat terapi alternatif bekam.
Human Heart Disease Prediction System Using Data Mining Techniques
Authors: Javed Sidra , Javed Hamza , Saddique Ayesha , Rafiq Beenish 
Published: June 2019

— Prediction of heart disease is a big concern now a days because everyone is busy and due to heavy load of work people do not give attention to their health. To diagnose a disease is a big challenge. The issue is to extract data that have some meaningful knowledge. For this purpose, data mining techniques are used to extract meaningful data. Decision Tree and ID3 are used to predict heart diseases. Many researchers and practitioners are familiar with prediction of heart diseases and wide range of techniques is available to predict disease. To address this problem, Decision Tree is used to predict the heart disease. In this study the collected data is pre-processed, Decision Tree algorithm and ID3 were then applied to predict the heart disease.

Index Terms— Decision Tree, ID3 Algorithm, Data Mining, Decision Support System (DSS), knowledge Discovery from Databases (KDD).
Spins of black holes in coalescing compact binaries
Authors: Postnov K A , Kuranov A G , Mitichkin N A 
Published: June 2019

Abstract
Modern astrophysical methods for determining spins of rotating stellar-mass black holes in close binaries and of supermassive black holes in active galactic nuclei are briefly discussed. Effective spins of coalescing binary black holes derived from LIGO/Virgo gravitational wave observations are specially addressed. The effective spins of coalescing astrophysical binary black holes and black holes with neutron stars are calculated for two plausible models of black hole formation from stellar core collapses (without or with an additional fallback from the stellar envelope) taking the stellar metallicity and star formation rate evolution in the Universe into account. The calculated distributions are consistent with the reported LIGO/Virgo observations. Distributions of the effective spins expected in yet undiscovered neutron star – black hole binaries have been calculated. The effective spins of primordial coalescing stellar-mass black holes can reach a few percent due to the accretion spin-up in a cold external medium.
PENGARUH SHOPPING LIFESTYLE DAN FASHION INVOLVEMENT TERHADAP IMPULSE BUYING BEHAVIOR
Authors: Fauziyyah Astri Nurrohmah , Oktafani Farah 
Published: June 2019

Perkembangan trend fashion yang semakin meningkat, menyebabkan kebutuhan manusia akan barang dan jasa pada bidang fashion semakin meningkat dan bervariasi. Para pelaku bisnis dituntut untuk menyediakan berbagai fashion yang menjadi selera konsumen. Dengan memerhatikan aspek shopping lifestyle dan fashion involvement para pelaku bisnis dapat menarik daya tarik konsumen dalam melakukan impulse buying behavior. Penelitian ini bertujuan untuk mengetahui shopping lifestyle dan fashion involvement terhadap impulse buying behavior pada masyarakat Kota Bandung. Pengambilan sampel dilakukan dengan teknik non-probability sampling dengan tipe sampling incidental yaitu teknik penentuan sampel berdasarkan kebetulan, yaitu siapa saja yang secara kebetulan bertemu dengan peneliti dengan jumlah responden sebanyak 400 responden. Teknik analisis yang digunakan yaitu analisis deskriptif dan analisis linear berganda.Berdasarkan hasil uji hipotesis secara parsial, shopping lifestyle dan fashion involvement terbukti berpengaruh secara signifikan terhadap impulse buying behavior, dan berdasarkan hasil uji hipotesis secara simultan shopping lifestyle dan fashion involvement berpengaruh secara simultan terhadap impulse buying behavior. Berdasarkan koefisien determinasi dapat disimpulkan bahwa besarnya pengaruh shopping lifestyle dan fashion involvement adalah sebesar 55,7%, sisanya sebesar 44,3% merupakan kontribusi dari variabel lain selain shopping lifestyle dan fashion involvement yang tidak diteliti dalam penelitian ini. Kata kunci: fashion involvement, impulse buying behavior, shopping lifestyle
SÍNDROME DE PINZAMIENTO DEL HOMBRO. Una Visión Desde la Perspectiva de la Fisioterapia.
Authors: Garita Meneses Geovanny 
Published: June 2019

En la actualidad, numerosos autores concuerdan en que las causas del llamado “Síndrome de Pinzamiento del Hombro” son multifactoriales. Estas se relación con eventos mecánicos que comprometen a los tejidos blandos subacromiales.
Algunos de los factores etiológicos comunes y que son más frecuentemente encontrados en la literatura son
•Traumas a repetición.
•Disminución de la actividad de la musculatura estabilizadora local (manguito rotador).
•Variación en la forma del acromion.
REINCIDENCIA EN LA CIRUGIA ESTÉTICA ASOCIADA A RASGOS DEL TRASTORNO DISMÓRFICO CORPORAL
Authors: Díaz Alvarado Susan Adriana 
Published: June 2019

La imagen corporal es la representación del cuerpo que cada persona construye en su mente y la vivencia que tiene sobresí mismo. Una cosa es la apariencia física y otra la imagen corporal. Personas con una apariencia física alejada de la norma de belleza pueden sentirse bien con su imagen corporal o de modo contrario.
Konflik Dalam Komunikasi Politik Antara Legislatif dan Eksekutif Dalam Menyikapi Rencana Tata Ruang dan Wilayah di Kabupaten Buton Selatan
Authors: Suherman Ansar 
Published: June 2019

Penelitian ini bertujuan untuk mengetahui pola hubungan komunikasi antara eksekutif dan legislatif beserta kendala dan masalah yang dihadapi dalam pelaksanaan kewenangan, serta bentuk konflik yang terjadi antara eksekutif dan legislatif dalam penyusunan Perda RTRW Kabupaten Buton Selatan.
Jenis Penelitian kualitatif dengan menggunakan purposive sampling, dimana data diperoleh melalui wawancara mendalam (depth interview) terhadap informan kunci (key informan) yang dianggap paham dengan tema penelitian. Data kemudian dianalisis menggunakan model komponensial (componential anaylisis).
Hasil penelitian menunjukkan bahwa pola hubungan komunikasi antara eksekutif dan legislatif dalam penyelesaian konflik dalam penetapan Perda RTRW Kabupaten Buton Selatan dilakukan melalui proses komunikasi organisasi formal dan komunikasi organisasi informal. Bentuk konflik yang terjadi antara eksekutif dan legislatif dalam penyusunan Perda RTRW Kabupaten Buton Selatana dalah konflik antar organisasi, yakni antara lembaga eksekutif dan legislatif Kabupaten Buton Selatan. Kendala yang dihadapi dalam pelaksanaan kewenangan dalam meningkatkan hubungan kerja antara eksekutif dan legislatif diantaranya adalah kerancuan data yang dituangkan eksekutif dalam draft Naskah Akademis RTRW dan kurangnya pemahaman legislatif terhadap RTRW sehingga tidak ada tanggapan kritis dari legislatif dalam perumusan ini. Sedangkan upaya untuk meningkatkan hubungan kerja antara eksekutif dan legislatif yaitu dengan mengesampingkan kepentingan-kepentingan individual dan mengutamakan kepentingan masyarakat.
SINERGI BIROKRASI, SWASTA DAN MASYARAKAT DALAM PROSES FORMULASI KEBIJAKAN PERENCANAAN PADA BAPPEDA DAN PENANAMAN MODAL KABUPATEN BUTON
Authors: Sadat Anwar 
Published: June 2019

Dalam konteks otonomi daerah, harapannya menjadi sarana terjadinya sinergi birokrasi, Swasta dan Masyarakat dalam Proses Formulasi Kebijakan Perencanaan pada Bappeda dan Penanaman Modal Kabupaten Buton. Tujuan penelitian ini adalah mengkaji proses formulasi kebijakan perencanaan pada Badan Perencanaan Pembangunan Daerah Kabupaten Buton dan peran para stakeholders dalam proses formulasi kebijakan perencanaan pada Bappeda dan Penanaman Modal Kabupaten Buton.
Penelitian ini menjelaskan bahwa Perencanaan menjadi katalisator pembangunan daerah yang didukung oleh masyarakat setempat, masyarakat memahami tentang kebijakan pemerintah dan dapat memperhitungkan kemampuannya dalam mendukung pembangunan daerah. Pola penyelenggaraan pemerintahan yang baik dalam era otonomi daerah tujuan mempromosikan good governance pada tingkat pemerintah daerah, melalui partisipasi publik dalam proses pengambilan kebijakan. Sampai sekarang belum terungkap bagaimana peran para stakeholders dalam proses perumusan kebijakan publik di Kabupaten Buton, disamping dapat berpengaruh terhadap sinergi para stakeholders dalam proses perumusan kebijakan pada Bappeda dan Penanaman Modal di kabupaten Buton.
REFORMASI PENEGAKAN HUKUM PERSPEKTIF HUKUM PROGRESIF
Authors: Ansori Lutfil 
Published: June 2019

This articel aim for examine reformation and optimalisation of law enforcement at law enforcerment institution in terms of progresive law perspective. the law face in Indonesia today is faced a complex problem on law enforcement process. Yet, Reformation on law enforcement is the answer to how the law in Indonesia is actuated within frame work of estabilishment an aspired state of law. Law enforcement reformation ideally must be done through legal system approach, that covered legal substance sub system, legal structure sub system, and legal culture subsystem. in the context of law enforcement institution reformation, institution reformation ideally based on three main orientation, which is democration principal, rule of law, and human rights. That institution reformation must be done with changing paradigm from the way of textual legal thinking to progresive legal thinking. It can be formed if reformation of law enforcement institution, consistent in bringing about changing cultural aspect that comes from changing structural aspect and instrumental aspect.
KEDUDUKAN AHLI WARIS YANG PENERIMA HIBAH DARI ORANG TUA TERHADAP AHLI WARIS LAINNYA PADA PROSES PEMBAGIAN WARIS
Authors: Sanjaya Umar Haris , Suprapton Muhammad Yusuf 
Published: June 2019

This research focused on the clarification in the meaning of legal status of the heir which is the heir received the donation (grant) from the parents before. In fact, the other heirs does not recognize the position of donation receiver to gets inheritance rights belong to parents. This research using context of probles as how the legal status of the heir (donation receiver) belong to the other heirs in receiving inheritance, is the donation receiver does not has rights in inheritance. Research result found that meaning of donation in the 3 perspective of private law giving the similar consequences, thus are based on private law (civil code), adat law, and islamic fiqih law (KHI). Those are giving perspective that donation is recognized as the inhertance. And the legal status of receiver donation is available to receive inheritance.
THE 7Be ii RESONANCE LINES IN TWO CLASSICAL NOVAE V5668 SGR AND V2944 OPH
Authors: Tajitsu Akito , Sadakane Kozo , Naito Hiroyuki , Arai Akira , Kawakita Hideyo , Aoki Wako 
Published: June 2019

ABSTRACT
We report spectroscopic observations of the resonance lines of singly ionized 7Be in the blueshifted absorption line systems found in the post-outburst spectra of two classical novae—V5668 Sgr (Nova Sagittarii 2015 No. 2) and V2944 Oph (Nova Ophiuchi 2015). The unstable isotope 7Be should have been created during the thermonuclear runaway (TNR) of these novae and decayed to form 7Li within a short period (a half-life of 53.22 days). These confirmations of 7Be are the second and the third ones following the first case found in V339 Del by Tajitsu et al. The blueshifted absorption line systems in both novae are clearly divided into two velocity components, both of which contain 7Be. This means that the absorbing gases in both velocity components consist of products of TNR. We estimated the amounts of 7Be produced during the outbursts of both novae and concluded that significant 7Li should have been created. These findings strongly suggest that the explosive production of 7Li via the reaction 3He(α,γ)7Be and its subsequent decay to 7Li occurs frequently among classical novae and contributes to the process of Galactic Li enrichment.
DISRUPTION OF MOLECULAR CLOUDS BY EXPANSION OF DUSTY H II REGIONS
Authors: Kim Jeong-Gyu , Kim Woong-Tae , Ostriker Eve C. 
Published: June 2019

ABSTRACT
Dynamical expansion of H ii regions around star clusters plays a key role in dispersing the surrounding dense gas and therefore in limiting the efficiency of star formation in molecular clouds. We use a semianalytic method and numerical simulations to explore expansion of spherical dusty H ii regions and surrounding neutral shells and the resulting cloud disruption. Our model for shell expansion adopts the static solutions of Draine for dusty H ii regions and considers the contact outward forces on the shell due to radiation and thermal pressures, as well as the inward gravity from the central star and the shell itself. We show that the internal structure we adopt and the shell evolution from the semianalytic approach are in good agreement with the results of numerical simulations. Strong radiation pressure in the interior controls the shell expansion indirectly by enhancing the density and pressure at the ionization front. We calculate the minimum star formation efficiency

required for cloud disruption as a function of the cloud’s total mass and mean surface density. Within the adopted spherical geometry, we find that typical giant molecular clouds in normal disk galaxies have

, with comparable gas and radiation pressure effects on shell expansion. Massive cluster-forming clumps require a significantly higher efficiency of

for disruption, produced mainly by radiation-driven expansion. The disruption time is typically of the order of a free-fall timescale, suggesting that the cloud disruption occurs rapidly once a sufficiently luminous H ii region is formed. We also discuss limitations of the spherical idealization.
DENSER SAMPLING OF THE ROSETTE NEBULA WITH FARADAY ROTATION MEASUREMENTS: IMPROVED ESTIMATES OF MAGNETIC FIELDS IN H ii REGIONS
Authors: Costa Allison H. , Spangler Steven R. , Sink Joseph R. , Brown Shea , Mao Sui Ann 
Published: June 2019

ABSTRACT
We report Faraday rotation measurements of 11 extragalactic radio sources with lines of sight through the Rosette Nebula, a prominent H ii region associated with the star cluster NGC 2244. The goal of these measurements is to better determine the strength and structure of the magnetic field in the nebula. We calculate the rotation measure (RM) through two methods, a least-squares fit to

χ
(

λ

2

)

and Rotation Measure Synthesis. In conjunction with our results from Savage et al., we find an excess RM due to the shell of the nebula of +40 to +1200 rad m−2 above a background RM of +147 rad m−2. We discuss two forms of a simple shell model intended to reproduce the magnitude of the observed RM as a function of distance from the center of the Rosette Nebula. The models represent different physical situations for the magnetic field within the shell of the nebula. The first assumes that there is an increase in the magnetic field strength and plasma density at the outer radius of the H ii region, such as would be produced by a strong magnetohydrodynamic shock wave. The second model assumes that any increase in the RM is due solely to an increase in the density, and the Galactic magnetic field is unaffected in the shell. We employ a Bayesian analysis to compare the two forms of the model. The results of this analysis were inconclusive, although the model without amplification of the interstellar magnetic field is weakly favored.
SIMULATIONS OF THE MG ii K AND CA ii 8542 LINES FROM AN ALFVÉN WAVE-HEATED FLARE CHROMOSPHERE
Authors: Kerr Graham S. , Fletcher Lyndsay. , Russell Alexander J. B. , Allred Joel C. 
Published: June 2019

ABSTRACT
We use radiation hydrodynamic simulations to examine two models of solar flare chromospheric heating: Alfvén wave dissipation and electron beam collisional losses. Both mechanisms are capable of strong chromospheric heating, and we show that the distinctive atmospheric evolution in the mid-to-upper chromosphere results in Mg ii k-line emission that should be observably different between wave-heated and beam-heated simulations. We also present Ca ii 8542 Å profiles that are formed slightly deeper in the chromosphere. The Mg ii k-line profiles from our wave-heated simulation are quite different from those from a beam-heated model and are more consistent with Interface Region Imaging Spectrograph observations. The predicted differences between the Ca ii 8542 Å in the two models are small. We conclude that careful observational and theoretical study of lines formed in the mid-to-upper chromosphere holds genuine promise for distinguishing between competing models for chromospheric heating in flares.
O vi EMISSION IMAGING OF A GALAXY WITH THE HUBBLE SPACE TELESCOPE: A WARM GAS HALO SURROUNDING THE INTENSE STARBURST SDSS J115630.63+500822.1∗
Authors: Hayes Matthew , Melinder Jens , Östlin Göran , Scarlata Claudia , Lehnert Matthew D. , Mannerström-Jansson Gustav 
Published: June 2019

ABSTRACT
We report results from a new Hubble Space Telescope campaign that targets the O vi

Å doublet in emission around intensely star-forming galaxies. The program aims to characterize the energy balance in starburst galaxies and gas cooling in the difficult-to-map coronal temperature regime of

K. We present the first resolved image of gas emission in the O vi line. Our target, SDSS J115630.63+500822.1, is very compact in the continuum but displays O vi emission to radii of 23 kpc. The surface brightness profile is well fit by an exponential with a scale length of 7.5 kpc. This is 10 times the size of the photoionized gas, and we estimate that about 1/6 the total O vi luminosity comes from resonantly scattered continuum radiation. Spectroscopy—which closely resembles a stacked sample of archival spectra—confirms the O vi emission, and determines the column density and outflow velocity from blueshifted absorption. The combination of measurements enables a large number of calculations with few assumptions. The O vi regions fill only

of the volume. By comparing the cooling time with the cloud sound-crossing time, the cooling distance with the size, and the pressure in the O vi and nebular gas, we conclude that the O vi-bearing gas cannot have been lifted to the scale height at this temperature, and must be cooling in situ through this coronal temperature regime. The coronal phase contains ∼1% of the ionized mass, and its kinetic energy at a given instant is ∼1% of the budget set by supernova feedback. However, a much larger amount of the gas must have cooled through this phase during the star formation episode. The outflow exceeds the escape velocity and the gas may become unbound, but it will recombine before it escapes and become visible to Lyman (and O i) spectroscopy. The mapping of this gas represents a crucial step in further constraining galaxy formation scenarios and guiding the development of future astronomical satellites.
THE REDSHIFTED HYDROGEN BALMER AND METASTABLE He i ABSORPTION LINE SYSTEM IN MINI-FELOBAL QUASAR SDSS J112526.12+002901.3: A PARSEC-SCALE ACCRETION INFLOW?
Authors: Shi Xi-Heng , Jiang Peng , Wang Hui-Yuan , Zhang Shao-Hua , Ji Tuo , Liu Wen-Juan , Zhou Hong-Yan 
Published: June 2019

ABSTRACT
The accretion of the interstellar medium onto central super-massive black holes is widely accepted as the source of the gigantic energy released by the active galactic nuclei. However, few pieces of observational evidence have been confirmed directly demonstrating the existence of the inflows. The absorption line system in the spectra of quasar SDSS J112526.12+002901.3 presents an interesting example in which the rarely detected hydrogen Balmer and metastable He i absorption lines are found redshifted to the quasar's rest frame along with the low-ionization metal absorption lines Mg ii, Fe ii, etc. The repeated SDSS spectroscopic observations suggest a transverse velocity smaller than the radial velocity. The motion of the absorbing medium is thus dominated by infall. The He i* lines present a powerful probe to the strength of ionizing flux, while the Balmer lines imply a dense environment. With the help of photoionization simulations, we find that the absorbing medium is exposed to the radiation with ionization parameter U ≈ 10−1.8, and the density is

. Thus the absorbing medium is located ∼4 pc away from the central engine. According to the similarity in the distance and physical conditions between the absorbing medium and the torus, we strongly propose the absorption line system as a candidate for the accretion inflow, which originates in the inner surface of the torus.