bluuebunny/crossref_metadata_2025_split huggingface dataset:
Carola Trips & Jaklin Kornfilt (eds.) (2017), "Further Investigations into the Nature of Phrasal Compounding", Berlin: Language Science Press
Authors: Hacken Pius ten 
Published: October 2018

Phrasal compounding is a phenomenon illustrated by slept all day look. Prototypical examples are determinative compounds with a nominal head and a phrasal non-head. They raise interesting questions about the interaction of syntax and morphology and have been discussed in this context by Botha (1981) for Afrikaans and Lieber (1992) for English. Also in German and Turkish, they have received ample attention. This volume has as its main purpose to extend the range of languages for which phrasal compounds are discussed. It consists of a brief introduction (chapter 1), six chapters devoted to individual languages, and a final chapter with a more general outlook. The use of further in the title is perhaps surprising, in particular because the volume under review is the first of a new series. It is motivated by the fact that the papers are from “the second workshop on phrasal compounding”, held in Mannheim in 2015. In this review, I will first present and discuss each chapter, then consider some general points about the volume.

Dieser Beitrag ist ursprünglich im Peter-Lang-Verlag erschienen (https://www.ingentaconnect.com/contentone/plg/jwf/2018/00000002/00000001/art00009)
Nicolaus Janos Raag: Substantivkomposita und Sinngebung im Kontext frühmittelalterlicher Wissensvermittlung. Eine kulturanalytisch­-linguistische Untersuchung zur Wortbildung bei Notker III
Authors: Stricker Stefanie 
Published: October 2018

Die hier zu besprechende Dissertation des schwedischen Germanisten Nicolaus Janos Raag ist an der Universität Uppsala (Schweden) unter der Betreuung von Dessislava Stoeva-Holm entstanden. Die Arbeit will zeigen, welche Rolle Substantivkomposita im Rahmen der Wissensvermittlung und des Kulturtransfers spielen, wie deutsche Komposita lateinisch vermittelte Inhalte in die eigene frühmittelalterliche klösterliche Kultur der Rezipienten integrieren und welche Veränderungen sie dabei erfahren. Für die Untersuchung wurden Substantivkomposita ausgewählt, da sie prädestiniert für die Benennung von bisher Unbekanntem sind und durch ihre binäre Struktur die Fähigkeit besitzen, zwei Größen zueinander in Beziehung zu setzen, wobei die semantische Relation zwischen den Konstituenten eines Kompositums prinzipiell offen und auf morphologischer Ebene nicht ausgedrückt ist.

Dieser Beitrag ist ursprünglich im Peter-Lang-Verlag erschienen (https://www.ingentaconnect.com/contentone/plg/jwf/2018/00000002/00000001/art00010)
How Does the Stellar Wind Influence the Radio Morphology of a Supernova Remnant?
Authors: Zhang M. F. , Tian W. W. , Wu D. 
Published: October 2018

Abstract
We simulate the evolution of the stellar wind and the supernova remnant (SNR) originating from a runaway massive star in a uniform Galactic environment based on three-dimensional magnetohydrodynamics models. Taking the stellar wind into consideration, we can explain the radio morphologies of many SNRs. The directions of the kinematic velocity of the progenitor, the magnetic field, and the line of sight are the most important factors influencing the morphologies. If the velocity is perpendicular to the magnetic field, the simulation will give us two different unilateral SNRs and a bilateral symmetric SNR. If the velocity is parallel to the magnetic field, we obtain a bilateral asymmetric SNR and a quasi-circular SNR. Our simulations show the stellar wind plays a key role in the radio evolution of an SNR, which implies that the Galactic global density and magnetic field distribution play a secondary role.
Modulation of Ion and Electron Pitch Angle in the Presence of Large-amplitude, Low-frequency, Left-hand Circularly Polarized Electromagnetic Waves Observed by MMS
Authors: Zhao J. S. , Wang T. Y. , Dunlop M. W. , He J. S. , Dong X. C. , Wu D. J. , Khotyaintsev Yu. V. , Ergun R. E. , Russell C. T. , Giles B. L. , Torbert R. B. , Burch J. L. 
Published: October 2018

Abstract
Most studies on low-frequency electromagnetic cyclotron waves have assumed a small wave amplitude, which ensures the reasonable application of linear and quasi-linear theories. However, the topic of large-amplitude electromagnetic cyclotron waves has not received much attention. Using Magnetospheric Multiscale measurements, this study observes low-frequency, left-hand circularly polarized electromagnetic waves with magnetic fluctuation ∼1–2 nT in the dusk flank side of the Earth’s magnetosheath. Considering the ambient magnetic field ∼15 nT therein, the relative wave amplitude is of the order of 0.1. These large magnetic field fluctuations result in a periodic variation of the ion pitch angle. The electron pitch angle exhibits a localized distribution feature with a timescale approximating the wave period. Moreover, some electrons are trapped at a pitch angle ∼90°, and the trapping is more remarkable as strong waves arise. These two features of the electron pitch angle distribution imply that the trapping of electrons (partly) results from large-amplitude electromagnetic cyclotron fluctuations. Our results illustrate the important role of large-amplitude electromagnetic cyclotron waves on the dynamics of charged particles.
The Ultraviolet Colors of Type Ia Supernovae and Their Photospheric Velocities
Authors: Brown Peter J. , Perry Jonathan M. , Beeny Britton A. , Milne Peter A. , Wang Xiaofeng 
Published: October 2018

Abstract
We compare ultraviolet (UV) and optical colors of a sample of 29 type Ia supernovae (SNe Ia) observed with the Swift satellite’s UltraViolet Optical Telescope with theoretical models of an asymmetric explosion viewed from different angles from Kasen & Plewa. This includes mid-UV (1600–2700 Å; uvw2 and uvm2) and near-UV (2700–4000 Å; uvw1 and u) filters. We find the observed colors to be redder than the model predictions, and that these offsets are unlikely to be caused by dust reddening. We confirm that high-velocity SNe Ia have red UV-optical observed colors. After correcting the colors for dust reddening by assuming a constant b − v color, we find no correlation between the uvw1 − v or u − v colors and the ejecta velocities for 25 SNe Ia with published velocities and/or spectra. When assuming an optical color–velocity relation, weak correlations of 2 and 3.6σ are found for uvw1 − v and u − v. However, we find that weak correlations can be reproduced with shuffled velocities and colors that are corrected for reddening. The slope and significance of a correlation between the UV colors and the velocity is thus dependent on the slope of the optical color–velocity relation. Even with a correction, a significant scatter still remains in the uvw1 − v colors including a large spread at low velocities, demonstrating that the NUV-blue/red spread is not caused by the photospheric velocity. The uvm2 − uvw1 colors also show a large dispersion uncorrelated with the velocity.
Circumnuclear Multiphase Gas in the Circinus Galaxy. II. The Molecular and Atomic Obscuring Structures Revealed with ALMA
Authors: Izumi Takuma , Wada Keiichi , Fukushige Ryosuke , Hamamura Sota , Kohno Kotaro 
Published: October 2018

Abstract
We used the Atacama Large Millimeter/Submillimeter Array (ALMA) to map the CO(3–2) and [C i](1–0) lines, as well as their underlying continuum emission, from the central ∼200 pc region of the Circinus galaxy that hosts the nearest type 2 Seyfert-class active galactic nucleus (AGN), with a spatial resolution of ∼6–15 pc. The lines and continuum-emitting regions consist of a circumnuclear disk (CND; 74 pc × 34 pc) and spiral arms. The distribution of the continuum emission revealed a temperature-dependent dust geometry and possibly polar dust elongation in the torus region. The molecular mass of the CND is

, with a beam-averaged H2 column density of ∼5 × 1023 cm−2 toward the AGN position, which contributes significantly to the nuclear obscuration. The [C i](1–0)/CO(3–2) ratio at the AGN position is unusually high, suggesting an X-ray-dominated region-type chemistry. We decomposed the observed velocity fields into rotational and dispersion components, and revealed a multiphase dynamic nature in the r ≲ 10 pc torus region, i.e., the diffuse atomic gas is more spatially extended along the vertical direction of the disk than the dense molecular gas. Through comparisons with our model predictions based on the radiation-driven fountain scheme, we indicate that atomic outflows are the driver of the geometrical thickness of the atomic disk. This supports the validity of the radiation-driven fountain scheme in the vicinity of this AGN, which would explain the longstanding mystery of the physical origin of the AGN torus.
Prompt Emission of Gamma-Ray Bursts from the Wind of Newborn Millisecond Magnetars: A Case Study of GRB 160804A
Authors: Xiao Di , Peng Zong-kai , Zhang Bin-Bin , Dai Zi-Gao 
Published: October 2018

Abstract
In this paper, we revisit the scenario that an internal gradual magnetic dissipation taking place within the wind from a newborn millisecond magnetar can be responsible for gamma-ray burst (GRB) production. We show that a combination of two emission components in this model, i.e., the photospheric emission from the wind and the synchrotron radiation within the magnetic reconnection region, can give a reasonable fit to the observed spectrum of the prompt emission phase of GRB 160804A. We obtain the physical parameters through a Monte Carlo procedure and deduce the initial spin period and magnetic field of the central magnetar. Furthermore, the independent afterglow fitting analysis gives a consistent result, adding great credibility to this scenario. In addition, we predict a subclass of GRBs from such Magnetar wind Internal Gradual MAgnetic Dissipation (abbreviated as “MIGMAD bursts”) that have several distinctive properties.
The MOSDEF Survey: Stellar Continuum Spectra and Star Formation Histories of Active, Transitional, and Quiescent Galaxies at 1.4 < z < 2.6
Authors: Zick Tom O. , Kriek Mariska , Shapley Alice E. , Reddy Naveen A. , Freeman William R. , Siana Brian , Coil Alison L. , Azadi Mojegan , Barro Guillermo , Fetherolf Tara , Fornasini Francesca M. , de Groot Laura , Leung Gene , Mobasher Bahram , Price Sedona H. , Sanders Ryan L. , Shivaei Irene 
Published: October 2018

Abstract
Using the MOSFIRE Deep Evolution Field (MOSDEF) rest-frame optical spectroscopic survey, we investigate the star formation histories (SFHs) of different galaxy types, ranging from actively star-forming to quiescent at 1.4 ≤ z ≤ 2.6. SFHs are constrained utilizing stellar continuum spectroscopy, specifically through a combination of Balmer absorption lines, the 4000 Å break, and the equivalent width of the Hα emission line. To attain a sufficiently high signal-to-noise ratio (S/N) to conduct these measurements we stack spectra of galaxies with similar spectral types, as determined from their rest-frame U − V and V − J colors. We bin the MOSDEF sample into five spectral types, subdividing the quiescent and star-forming bins to better explore galaxies transitioning between the two. We constrain the average SFHs for each type, finding that quiescent and transitional galaxies in the MOSDEF sample are dominated by an SFH with an average star formation timescale of τ ∼ 0.1–0.2 Gyr. These findings contrast with measurements from the low-redshift Universe where, on average, galaxies form their stars over a more extended time period (τ > 1 Gyr). Furthermore, our spectral index measurements correlate with mass surface density for all spectral types. Finally, we compare the average properties of the galaxies in our transitional bins to investigate possible paths to quiescence, and speculate on the viability of a dusty post-starburst phase.
SOFIA FIFI-LS Observations of Sgr B1: Ionization Structure and Sources of Excitation
Authors: Simpson Janet P. , Colgan Sean W. J. , Cotera Angela S. , Kaufman Michael J. , Stolovy Susan R. 
Published: October 2018

Abstract
The current paradigm of Galactic Center (GC) gas motions and star formation envisions sequential star formation in streams of gas as they pass near the supermassive black hole Sgr A*. This is based on the relative positions of dense molecular clouds, the very young star-forming region Sgr B2, the much older region Sgr C, and the several Myr old Arches and Quintuplet Clusters. Because Sgr B1 is found with Sgr B2 in a common envelope of molecular gas and far-infrared emission, the two sources are thought to be physically related, even though there are indicators of a significantly greater age for Sgr B1. To clarify the status of Sgr B1, we have mapped it with the FIFI-LS spectrometer on the Stratospheric Observatory for Infrared Astronomy in the far-infrared lines of [O iii] 52 and 88 μm. From the ratios of these lines and lines measured with the Spitzer Infrared Spectrograph, we find that there are at least eight separate sub-regions that must contain the stars that excite the gas. We infer spectral energy distributions (SEDs) of the ionizing sources from models and find they are in agreement only with SEDs of late O stars augmented at the highest frequencies with interstellar X-rays from fast shocks. We suggest that although the gas, from its velocity structure, must be part of the very young Sgr B2 complex, the stars that are ionizing the gas were not formed there but are the remnants of a previous generation of star formation in the GC.
A list of bees from three locations in the Northern Rockies Ecoregion (NRE) of western Montana
Authors: Reese Elizabeth , Burkle Laura , Delphia Casey , Griswold Terry 
Published: October 2018

Wild bees that were collected in conjunction with a larger study are presented as a checklist of species for the Northern Rockies Ecoregion of Montana, USA. Over the course of four field seasons (2013-2016), 281 species and morphospecies in 32 genera and five families were collected using insect nets, and identified. This paper addresses the distinct lack of studies monitoring bee species in Montana and contributes to a basic understanding of fauna in the northern Rocky Mountains.With this study, the number of known bee species in Montana increases by at least six species, from 366 (Kuhlman and Burrows 2017) to 372. Though literature was not reviewed for all the species on this checklist, published records in Montana revealed no listings forAndrenasaccataViereck;Anthidiellumnotatumrobertsoni(Cockerell);Ashmeadiellameliloti(Cockerell);Ashmeadiellapronitens(Cockerell);ColleteslutzilutziTimberlake; andDioxysproductus(Cresson).
New Nurses' Positive Evaluation of Transition-to-Practice Programs
Authors: Smyth Wendy , Pianta Paula , Perkins Rosemary 
Published: October 2018

Background:
The established nurse transition-to-practice program offered at one Australian health service underwent significant changes in 2017. This study aimed to gain feedback from the participants in the 2016 and 2017 programs.

Method:
A four-page paper survey was given to participants in the 2016 and 2017 programs.

Results:
Both cohorts were positive about the content, organization, and support provided to them throughout the program.

Conclusion:
The program will continue to undergo incremental improvements to meet the needs of the organization and the graduates. The need to tailor future programs to meet the needs of nurses working in rural and remote facilities has been identified. It has been suggested that options for more dynamic presentations of content also need to be explored.

J Contin Educ Nurs.
2018;49(11):500–506.
Nurses' Use of Appropriate Needle Sizes When Administering Intramuscular Injections
Authors: White Sheila , Goodwin John , Mgmt Dip , Behan Laura 
Published: October 2018

Background:
In cases where patients are overweight or obese, administration of intramuscular medications can be ineffective due to inappropriate sizes of needles used. This study investigated whether the size of needles used to administer intramuscular injections is appropriate for patients on the basis of their weight or body mass index.

Method:
This retrospective review examined 100 instances of intramuscular injection on a 50-bed ward.

Results:
In most instances, intramuscular medication was inappropriately administered. Needle sizes were not determined based on body mass index, and the possibility of true intramuscular penetration was minimal. Appropriate needle sizes were more likely to be chosen when instructions were provided with medications.

Conclusion:
Current available needle sizes may be inappropriate for certain patients. Nursing staff require further education to assist them in making correct needle choices. It is also important that health care settings have evidence-based policies in place and the necessary resources provided to ensure safe and correct administration of medication.

J Contin Educ Nurs.
2018;49(11):519–525.
Normal Intraocular Pressure in Children
Authors: Pensiero Stefano , Da Pozzo Stefano , Perissutti Paolo , Cavallini Gian Maria , Guerra Roberto 
Published: October 2018

ABSTRACT
The age-related trend values and the normal intraocular pressure (IOP) increase curve from birth through the 16th year of life were studied in 460 subjects with a noncontact tonometer (Keeler Pulsair, Keeler, Ltd, Windsor, Berks, UK). Much lower values than in adults were recorded in subjects up to the age of 3 or 4 years. This finding leads us to believe that in the treatment of infantile glaucoma IOP should be kept within the age physiologic levels, in an attempt to prevent visual field loss and optic atrophy.
Détermination de la peine et dilemmes éthiques dans le système de justice des mineurs : comprendre la prise de décision des acteurs judiciaires
Authors: Linteau Isabelle , Leclerc Chloé , Lafortune Denis 
Published: October 2018

La détermination de la peine chez les adolescents contrevenants est un processus complexe pouvant parfois soulever des dilemmes éthiques. L’objectif de cette étude est de mieux comprendre la prise de décision des acteurs judiciaires en pareilles circonstances. Pour ce faire, des entretiens semi-dirigés ont été menés auprès d’un échantillon de 30 acteurs judiciaires. Après avoir décrit un dilemme éthique vécu lors de leur pratique judiciaire, des procureurs de la Couronne et des délégués à la jeunesse étaient invités à expliquer comment ils avaient tranché leur dilemme. L’analyse des dilemmes racontés par ces acteurs révèle que ces derniers portent majoritairement sur les fondements même de la peine : devaient-ils recommander au tribunal une peine juste, qui rendrait bien compte de la gravité du crime commis, ou devaient-ils plutôt recommander une peine utile, qui répondrait aux besoins du jeune (en termes de réhabilitation) et aux besoins de la société (en termes de prévention de la récidive) ? L’analyse des motifs évoqués par les acteurs judiciaires pour justifier leur décision finale montre comment le choix d’une approche (juste dû, utilitarisme ou position intermédiaire) teinte l’analyse qu’ils font des différents éléments du dossier et le sens qu’ils donnent à ces éléments.
Déjouer les relations de genre. L’art bouffon de la mixité au Mali
Authors: Carbonnel Laure 
Published: October 2018

Que devient le genre dans les mains des bouffons rituels kɔrɔduga (korèduga) ? L’art bouffon de jouer avec la mixité sexuelle sera appréhendé à partir de situations d’interlocutions parlées et chantées. Trois modalités de déjouer les rapports de genre sont présentées. La première est la transversalité qui dissipe la division sexuelle (et sociale) des tâches extrêmement prégnantes dans la vie quotidienne. La seconde modalité déjoue les relations statutaires entre hommes et femmes, en inversant le rapport entre statut et activité. Enfin, les performances chantées de l’ensemble des bouffons rituels montrent également le rôle important de l’adresse indirecte pour que des paroles subversives puissent être entendues.
Les Azriat des Aurès, entre émancipation et injonctions nationales
Authors: Ramdani Karima 
Published: October 2018

Cet article s’intéresse au statut de femmes libres, les Azriat, durant la colonisation française en Algérie. Les Azriat exerçaient le métier de chanteuses et de danseuses dans l’Est de l’Algérie, dans une région appelée les Aurès. Ces artistes étaient des femmes veuves, divorcées ou répudiées jouissant d’une certaine liberté économique et sexuelle. À l’époque coloniale, leur mode de vie était condamné par les colons qui voyaient en elles l’illustration parfaite d’une société « indigène » décadente, mais il l’était aussi par des mouvements nationalistes occupés à façonner une image de ce que serait la femme algérienne idéale. Les Azriat étaient pourtant tolérées et même honorées par leur communauté car elles étaient perçues comme des artistes à part entière que l’on invitait pour différentes occasions. Cet article étudie la façon dont l’image de ces femmes a été utilisée, dans certaines circonstances, pour créer des frontières racialisées entre colons et « indigènes ». L’analyse de leurs performances artistiques permet également d’interroger une forme atypique de subjectivation et de transgression des normes de genre et de « race », et de rendre audibles les expériences de ces sujets pris dans différents rapports de domination.
Mesoscale fine structure of a tropopause fold over mountains
Authors: Woiwode Wolfgang , Dörnbrack Andreas , Bramberger Martina , Friedl-Vallon Felix , Haenel Florian , Höpfner Michael , Johansson Sören , Kretschmer Erik , Krisch Isabell , Latzko Thomas , Oelhaf Hermann , Orphal Johannes , Preusse Peter , Sinnhuber Björn-Martin , Ungermann Jörn 
Published: October 2018

Abstract. We report airborne remote-sensing observations of a tropopause fold during
two crossings of the polar front jet over northern Italy on 12 January 2016.
The GLORIA (Gimballed Limb Observer for Radiance Imaging of the Atmosphere)
observations allowed for a simultaneous mapping of temperature, water vapour,
and ozone. They revealed deep, dry, and ozone-rich intrusions into the
troposphere. The mesoscale fine structures of dry filaments at the cyclonic
shear side north of the jet and tongues of moist air entraining tropospheric
air into the stratosphere along the anticyclonic shear side south of the jet
were clearly resolved by GLORIA observations. Vertically propagating mountain
waves with recorded temperature residuals exceeding ±3 K were detected
above the Apennines. Their presence enhanced gradients of all variables
locally in the vicinity of the tropopause. The combination of
H2O−O3 correlations with potential temperature reveals an active
mixing region and shows clear evidence of troposphere-to-stratosphere and
stratosphere-to-troposphere exchange. High-resolution short-term
deterministic forecasts of ECMWF's integrated forecast system (IFS) applying
GLORIA's observational filter reproduce location, shape, and depth of the
tropopause fold very well. The fine structure of the mixing region, however,
cannot be reproduced even with the 9 km horizontal resolution of the
IFS, used here. This case study demonstrates convincingly the capabilities of linear
limb-imaging observations to resolve mesoscale fine structures in the upper
troposphere and lower stratosphere, validates the high quality of the IFS
data, and suggests that mountain wave perturbations have the potential to
modulate exchange processes in the vicinity of tropopause folds.