bluuebunny/crossref_metadata_2025_split huggingface dataset:
Hubungan Faktor Demografi dan Perilaku Seksual Terhadap Kejadian Infeksi Menular Seksual pada Wanita Pekerja Seks
Authors: Fitriasih Yuli , Fitriasih Yuli , Shahib Nurhalim , Husin Farid 
Published: October 2019

Abstract
Sexually transmitted infections are infections that can be spread through vaginal, anal or oral. Female sex workers particularly at risk for sexually transmitted infections. Preliminary studies in Cilacap district STI clinic in 2011 showed that the incidence of sexually transmitted infections is still quite high (60.81%). Complex causal factors cause the difficulty of breaking the chain of IMS. This study aims to analyze the relationship between demographic factors and high-risk sexual behavior of high risk on the incidence of sexually transmitted infections and the risk factors on the incidence of sexually transmitted infections in female sex workers. Analytic survey research through case-control study (case-control) with a total sampling on 70 female sex workers in brothels Slarang conducted during the month of November 2013. Questionnaire as a means of collecting research data. Univariate analysis to determine the frequency distribution of incidence of STIs. Bivariate analysis using contingency coefficient test. Multivariate analysis using logistic regression. The results showed that there is a significant association between the incidence of STIs in high- risk demographic factors with r value (0.239) and p-value (0.040), there is a significant association between the incidence of STIs in high- risk sexual behavior factors with values â€‹â€‹of r (0.307; 0.230) and the p-value ( 0.007; 0.048) respectively. Multivariate analysis showed that condom use is not routine is that most risk factors on the incidence of sexually transmitted infections in female sex workers with OR value 5.835. Conclusions of the study: female sex workers who do not regularly use condoms have 5.835 times greater risk for sexually transmitted infections. A total of 65% the proportion of female sex workers suffer preventable sexually transmitted infection, if condom use.
Keywords : female sex workers, demographic factors, sexual behavior factors, sexually transmitted infections
Optimasi sediaan salep minyak cengkeh (syzigium aromaticum) dalam basis larut air
Authors: Prabandari Rani 
Published: October 2019

Abstract

The clove flower essential oil (Syzygium aromaticum) with the active compound eugenol has been widely investigated and is known to be efficacious as an anti-inflammatory agent, and further research on its formulation continues. The formula developed in this study was a topical ointment dosage form using a water soluble base (oleic acid enhancer and propylene glycol). This study aims to determine the physical and irritant properties of the clove flower essential oil ointment (MABC) if a hydrocarbon base is used. The ointment is made by the smelting method with a concentration of 5% (F1), 10% (FII) and 15% (FIII). The ointments of the three formulas were then evaluated for their physical properties, including dispersion, adhesion and pH. The results of statistical tests with the LSD test showed that there were significant differences between formulas. The higher the concentration of MABC, the greater the spread (p0.05). The results of the Simplex Lattice Design irritation test also show that water-soluble base ointment with a concentration of 5%, 10% and 15% MABC does not cause an irritating effect.

Keywords: Syzygium aromaticum, base of water soluble ointment, anti-inflammatory.
STUDI PENGARUH STATUS PERKAWINAN DAN PEKERJAAN PADA PASIEN TUBERKULOSIS DI RUMAH SAKIT DKT PURWOKERTO
Authors: Octaviani Peppy 
Published: October 2019

ABSTRACT
Pulmonary tuberculosis (TB) is a contagious pulmonary infectious disease that is still a health problem in the world, especially developing countries. Tuberculosis has been proclaimed by WHO (World Health Organization) as Global Emergency since 1992. The purpose of this study is to find out what physical characteristics are at risk of tuberculosis in DKT Hospital Purwokerto. The research design used in this study was a descriptive study with a cross-sectional approach to determine the characteristics of pulmonary TB patients who were adherent to treatment and those who did not comply with treatment at the DKT Hospital in Purwokerto. This research was conducted at the DKT Purwokerto Hospital in May 2018. The samples studied in this study were pulmonary TB patients who were obedient to treatment and non-compliance with treatment at the DKT Purwokerto Hospital for the period of 1 January - 30 December 2017 that met the sample criteria. The results of the study have no relationship between age and the results of sputum examination at the Purwokerto DKT Hospital (p value = 0.286), there is no relationship between sex with the results of sputum examination at DKT Purwokerto Hospital (p value = 0.261).

Keywords: Pulmonary TBC, Characteristics, Phlegm Examination
PENGARUH USIA DAN JENIS KELAMIN PADA KEPATUHAN PASIEN DIABETES MELITUS MENGGUNAKAN OBAT ANTIDIABETES DI PERUM KETAPANG SOKARAJA KULON
Authors: Kusuma Ikhwan Yuda 
Published: October 2019

ABSTRACT
The WHO survey results show that the number of DM patients in Indonesia is ranked the 4th largest in the world. DM causes death by 5% every year. Deaths from DM are expected to increase by 50% in the next ten years. The results of the 2007 Central Java RISKESDAS showed that the prevalence of DM in Central Java province was 0.8% and overall was 1.3%. The highest prevalence is found in Cilacap Regency (3.9%), second place is Tegal City Regency (3.1%), for the third place is Surakarta (2.8%), fourth place is Pemalang (2.1%), and fifth place is occupied by Banyumas (1.9%) (Ministry of Health, 2009). This study used an experimental design by treating the group of cases. The research instruments in this study were interview guides about the number of remaining antidiabetic drugs to check the compliance and MMAS questionnaires that had been validated and translated into Indonesian versions (Setyaningsih, 2013). The results of data analysis using the Chi-Square test were obtained p = 0.220 (p> 0.05) based on the MMAS questionnaire, this indicates that this indicates that this study of age has a significant influence on the adherence of antidiabetic use in DM patients in Perum Ketapang Sokaraja Kulon.

Keywords: Age, Diabetes Mellitus, Drug Information
RECONSTRUCTION OF THE STAGE OF PREPARATION OF COMPOSITIONS OF ADDITIVES FOR LUBRICATING OILS
Authors: Scherbin Sergey 
Published: October 2019

Two options of reconstruction of knot of preparation of compositions of additives for
lubricant oils on JSC «ANHK» are considered. Comparison of the proposed technical solutions is executed and the conclusion is drawn on a possibility of their practical application by results of technical and economic calculations taking into account financial opportunities of the enterprise.
MODEL OF STRUCTURED DEMAND FOR INTERREGIONAL FORECASTING OF RAW OF GOODS
Authors: Lebedeva Ol'ga 
Published: October 2019

The article discusses the forecasting of commodity flows and factors affecting them,
the use of which will allow for a more accurate assessment of the demand for freight traffic for regional models. The main characteristics of land use and assessment of attractiveness are given.
The task of inter-regional forecasting the flow of commodities can be solved by implementing a
structured demand model. The choice of model and its variables depends on the nature of the available data on the transportation process
STUDY OF ELECTROMECHANICAL COMPLEXES WITH SYNCHRONOUS GENERATORS WITH DIFFERENT SYNCHRONIZATION MODES
Authors: Konovalov Yuriy , Sadovskiy Stepan , Krivosheev Maksim , Tihonova Angelina 
Published: October 2019

The results of experimental studies of various methods of synchronization of electromechanical complexes with synchronous generators arising when the synchronous generator is turned
on for parallel operation with the network and during self-synchronization during emergency modes
of a short circuit are presented.
IMPROVEMENT OF CHARACTERISTICS OF THE WIDE-PULSE INVERTER WHEN WORKING FOR ASYNCHRONOUS LOAD
Authors: Arsent'ev Grigoriy 
Published: October 2019

ь частоты, моделирование.
Abstract. The urgency of the problem of studying the operation of inverters in the frequency
Converter is shown. The characteristics of the pulse-width inverter when working on an asynchronous
load are obtained. According to the results of research, conclusions are made to determine the relationship between the form of output current and current in the DC voltage link and the mode of operation of the asynchronous motor. It is determined that the inverter has the greatest influence on the internal and output characteristics of the frequency Converter. the Converter has an inverter.
GENERAL APPROACH TO DESCRIPTION OF NONLINEAR DYNAMICS INTERACTION ON THE BOUNDARY OF PHASES GAS-SOLID
Authors: Sverdlova Ol'ga , Kondrat'eva Larisa 
Published: October 2019

The article presents a possible approach to the description of the nonlinear interaction on the boundary of phases in gas-solid. The study of interaction involves the construction of interconnected mathematical models of the procedure for ranking elementary stages in order of importance and. calculating the speed of the process of gas adsorption on heterogeneous surface of the
adsorbent. Submitted material should be seen as a statement of the general approach to the study of a
model example that allows practical implementation on a computer.
Constraining Mass-transfer Histories of Blue Straggler Stars with COS Spectroscopy of White Dwarf Companions
Authors: Gosnell Natalie M. , Leiner Emily M. , Mathieu Robert D. , Geller Aaron M. , Knigge Christian , Sills Alison , Leigh Nathan W. C. 
Published: October 2019

Abstract
Recent studies show that the majority of blue straggler stars (BSSs) in old open clusters are formed through mass transfer from an evolved star onto a main-sequence companion, resulting in a BSS and white dwarf (WD) in a binary system. We present constraints on the mass transfer histories of two BSS–WD binaries in the open cluster NGC 188, using WD temperatures and surface gravities measured with Hubble Space Telescope COS far-ultraviolet spectroscopy. Adopting a Gaia-based cluster distance of 1847 ± 107 pc, we determine that one system, WOCS 4540, formed through Case C mass transfer resulting in a CO-core WD with T
eff =

K and a log g =

, corresponding to a mass of

M
⊙ and a cooling age of

Myr. The other system, WOCS 5379, formed through Case B mass transfer resulting in a He-core WD with T
eff =

K and a log g =

, corresponding to a mass of

M
⊙ and an age of

Myr. The WD parameters are consistent across four different cluster distance assumptions. We determine possible progenitor binary systems with a grid of accretion models using MESA, and investigate whether these systems would lead to stable or unstable mass transfer. WOCS 4540 likely resulted from stable mass transfer during periastron passage in an eccentric binary system, while WOCS 5379 challenges our current understanding of the expected outcomes for mass transfer from red giant branch stars. Both systems are examples of the value in using detailed analyses to fine-tune our physical understanding of binary evolutionary processes.
The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion and Broad Emission Line Physics from a Hypervariable Quasar
Authors: Dexter Jason , Xin Shuo , Shen Yue , Grier C. J. , Liu Teng , Gezari Suvi , McGreer Ian D. , Brandt W. N. , Hall P. B. , Horne Keith , Simm Torben , Merloni Andrea , Green Paul J. , Vivek M. , Trump Jonathan R. , Homayouni Yasaman , Peterson B. M. , Schneider Donald P. , Kinemuchi K. , Pan Kaike , Bizyaev Dmitry 
Published: October 2019

Abstract
We analyze extensive spectroscopic and photometric data of the hypervariable quasar SDSS J141324+530527 (RMID 017) at z = 0.456, an optical “changing-look” quasar from the Sloan Digital Sky Survey Reverberation Mapping project that increased in optical luminosity by a factor ≃10 between 2014 and 2017. The observed broad emission lines all respond in luminosity and width to the changing optical continuum, as expected for photoionization in a stratified, virialized broad emission line region. The luminosity changes therefore result from intrinsic changes in accretion power rather than variable obscuration. The variability is continuous and apparently stochastic, disfavoring an origin as a discrete event such as a tidal disruption flare or microlensing event. It is coordinated on day timescales with blue leading red, consistent with reprocessing powering the entire optical spectral energy distribution. We show that this process cannot work in a standard thin disk geometry on energetic grounds, and would instead require a large covering factor reprocessor. Disk instability models could potentially also explain the data, provided that the instability sets in near the inner radius of a geometrically thick accretion disk.
Understanding Lyα Nebulae at Low Redshift. I. The Sizes, Powering, and Kinematics of “Green Bean” Galaxies
Authors: Prescott Moire K. M. , Sanderson Kelly N. 
Published: October 2019

Abstract
A new but rare sample of spatially extended emission line nebulae, nicknamed “Green Beans,” was discovered at z ≈ 0.3 thanks to strong [O iii] emission, and subsequently shown to be local cousins of the Lyα nebulae found at high redshift. Here we use follow-up APO/DIS spectroscopy to better understand how these low-redshift Lyα nebulae compare to other populations of strong emission line sources. Our spectroscopic data show that low-z Lyα nebulae have active galactic nucleus (AGN)-like emission line ratios, relatively narrow line widths (FWHM ≲ 1000 km s−1), and emission line kinematics resembling those of Type 2 AGN at the same redshift, confirming that they are powered by Type 2 AGN with typical ionizing continua. While low-z Lyα nebulae are larger and less concentrated than compact, star-forming Green Pea galaxies, we find that they resemble typical Type 2 AGN in terms of r-band concentration and size. Based on this pilot study, low-z Lyα nebulae appear to be a subset of Type 2 AGN with bluer optical continua and high [O iii] equivalent widths but with comparable sizes and similar [O iii] kinematics. These characteristics may simply reflect the fact that low-z Lyα nebulae are drawn from the high-luminosity end of the Type 2 AGN distribution, with higher nuclear activity driving higher [O iii] equivalent widths and more central star formation leading to bluer optical continua. Deeper spectroscopic follow-up of the full sample will shed further light on these issues and on the relationship between these low-z Lyα nebulae and the Lyα nebula population at high redshift.
Chandra Survey of Nearby Highly Inclined Disk Galaxies. V. Emission Structure and Origin of Galactic Coronae
Authors: Jiang Xiaochuan , Li Jiangtao , Fang Taotao , Wang Q. Daniel 
Published: October 2019

Abstract
The origin of the extended soft X-ray emission around nearby highly inclined disk galaxies (often called the X-ray corona) remains uncertain. The emission could arise from volume-filling hot gas and/or its interaction with cool gas. Morphological properties of the X-ray emission can provide additional information to distinguish these different origins. We define model-independent parameters H
50, H
75, and H
95—vertical scales that enclose 50%, 75%, and 95% of the total flux of the emission, respectively. We study the correlation of these parameters with galaxy properties inferred from infrared observations of a sample of nearby highly inclined disk galaxies with high-quality Chandra data. We find weak negative correlations between H
50 or H
75 and the surface star formation rate (I
SFR), and no correlation for H
95. However, we detect strong negative correlations of the vertical concentration of the emission, defined as H
50/H
95 or H
75/H
95, with I
SFR. Our findings suggest that the X-ray emission around disk galaxies is likely comprised of two components: the extended, weak emission, characterized by H
95, is influenced by the outflowing hot gas entrained in star formation driven winds, whereas the strong emission close to the disk, which is often rich in cool gas characterized by H
50 or H
75, is largely impacted by cool–hot gas interaction.
Pulsar Glitch Activity as a State-dependent Poisson Process: Parameter Estimation and Epoch Prediction
Authors: Melatos A. , Drummond L. V. 
Published: October 2019

Abstract
Rotational glitches in some rotation-powered pulsars display power-law size and exponential waiting-time distributions. These statistics are consistent with a state-dependent Poisson process, where the glitch rate is an increasing function of a global stress variable (e.g., crust-superfluid angular velocity lag), diverges at a threshold stress, increases smoothly while the star spins down, and decreases step-wise at each glitch. A minimal, seven-parameter, maximum likelihood model is calculated for PSR J1740−3015, PSR J0534+2200, and PSR J0631+1036, the three objects with the largest samples whose glitch activity is Poisson-like. The estimated parameters have theoretically reasonable values and contain useful information about the glitch microphysics. It is shown that the maximum likelihood, state-dependent Poisson model is a marginally (23%–27%) better post factum “predictor” of historical glitch epochs than a homogeneous Poisson process for PSR J1740−3015 and PSR J0631+1036 and a comparable predictor for PSR J0534+2200. Monte Carlo simulations imply that ≳50 glitches are needed to test reliably whether one model outperforms the other. It is predicted that the next glitch will occur at Modified Julian Date (MJD) 57,784 ± 256.8, 60,713 ± 1935, and 57,406 ± 1444 for the above three objects, respectively. The analysis does not apply to quasiperiodic glitchers like PSR J0537−6910 and PSR J0835−4510, which are not described accurately by the state-dependent Poisson model in its original form.
Four Newborn Planets Transiting the Young Solar Analog V1298 Tau
Authors: David Trevor J. , Petigura Erik A. , Luger Rodrigo , Foreman-Mackey Daniel , Livingston John H. , Mamajek Eric E. , Hillenbrand Lynne A. 
Published: October 2019

Abstract
Exoplanets orbiting pre-main-sequence stars are laboratories for studying planet evolution processes, including atmospheric loss, orbital migration, and radiative cooling. V1298 Tau, a young solar analog with an age of 23 ± 4 Myr, is one such laboratory. The star is already known to host a Jupiter-sized planet on a 24 day orbit. Here, we report the discovery of three additional planets—all between the sizes of Neptune and Saturn—based on our analysis of K2 Campaign 4 photometry. Planets c and d have sizes of 5.6 and 6.4

, respectively, and with orbital periods of 8.25 and 12.40 days reside 0.25% outside of the nominal 3:2 mean-motion resonance. Planet e is 8.7

in size but only transited once in the K2 time series and thus has a period longer than 36 days, but likely shorter than 223 days. The V1298 Tau system may be a precursor to the compact multiplanet systems found to be common by the Kepler mission. However, the large planet sizes stand in sharp contrast to the vast majority of Kepler multiplanet systems, which have planets smaller than 3

. Simple dynamical arguments suggest total masses of <28

and <120

for the c–d and d–b planet pairs, respectively. The implied low masses suggest that the planets may still be radiatively cooling and contracting, and perhaps losing atmosphere. The V1298 Tau system offers rich prospects for further follow-up including atmospheric characterization by transmission or eclipse spectroscopy, dynamical characterization through transit-timing variations, and measurements of planet masses and obliquities by radial velocities.
Floristic composition in ecotone forests in northern Brazilian Amazonia: preliminary data
Authors: Silva Williamar , Villacorta Carlos Darwin , Perdiz Ricardo , Farias Hugo , Oliveira Andressa , Citó Arthur , Carvalho Lidiany Camila , Barbosa Reinaldo 
Published: October 2019

Ecotone has been defined as “a multi-dimensional environmentally stochastic interaction zone between ecological systems with characteristics defined in space and time, and by the strength of the interaction” (Hufkens et al. 2009). This is a known concept to define transitional zones between two or more ecological communities, ecosystems or biotic regions. Ecotone forests, dispersed in northern Brazilian Amazonia, are natural formations which have been largely affected by anthropogenic impacts, such as deforestation and fire. Maracá Ecological Station, State of Roraima, Brazil, is a protected area with extensive representations of ecotone forests in this region of the Amazonia. Forest inventories and floristic surveys are important as they extend our knowledge (1) of forest structure and tree species composition and (2) of tree and palm species ecology in this region of the Amazonia. Both improve our ability to predict changes in plant diversity, considering the future scenarios of climate change in comparison with previous surveys performed in Maracá.
We present a forest inventory carried out in 129 plots (10 m x 50 m; 6.45 ha in total) dispersed in a grid (5 km x 5 km) located in a forest zone ecotone in the eastern part of Maracá Ecological Station. All stems (tree + palm) with diameter at breast height ≥ 10 cm were recorded, identified and measured. A total of 3040 stems were recorded (tree = 2815; palm = 225), corresponding to 42 botanic families and 140 identified species. Seven families and 20 genera contained unidentified taxa (12.2%). Sapotaceae (735 stems; 10 species), Leguminosae (409; 24) and Rubiaceae (289; 12) were the most abundant families. Peltogyne gracilipes Ducke (Leguminosae), Pradosia surinamensis (Eyma) T.D.Penn. (Sapotaceae) and Ecclinusa guianensis Eyma (Sapotaceae) were the species with the highest importance value index (~ 25%). The dominance (m2 ha-1) of these species corresponds to &gt; 36% of the total value observed in the forest inventory. Our dataset provides complementary floristic and structure information on tree and palm in Maracá, improving our knowledge of this Amazonian ecotone forest.
„Was nuw ist/ allzyt doren glust“. Alte und neue Welt in Brants Narrenschiff
Authors: Schillinger Jean 
Published: October 2019

La Nef des fous de Sebastian Brant porte la marque d’une opposition systématique entre le monde actuel et un monde passé, généralement idéalisé. Brant évoque une décadence universelle, qu’il voit à l’œuvre dans le domaine moral, politique, religieux et social. Il considère comme une forme de folie le goût de la nouveauté qui s’est emparé de ses contemporains et les pousse à rompre avec la tradition. Les nouvelles modes vestimentaires font l’objet d’une critique sévère, ainsi que les nouvelles pratiques économiques qui permettent le rapide enrichissement de certains au prix de l’appauvrissement de nombreux individus. Ces innovations mettent en cause l’ordre du monde et sont de nature à hâter la fin de celui-ci. De même, les innovations techniques et scientifiques suscitent la méfiance de Brant. Il est néanmoins difficile de déterminer l’attitude exacte de Brant, car de nombreux passages contredisent ses déclarations. D’autre part, la volonté didactique et l’engagement politique en faveur de Maximilien I er s’accordent mal avec l’affirmation fataliste d’un déclin irréversible.