bluuebunny/crossref_metadata_2025_split huggingface dataset:
Other ’68ers in West Berlin: Christian Democratic Students and the Cold War City
Authors: von der Goltz Anna 
Published: March 2017

AbstractMany of the most iconic moments of Germany's “1968” took place in the walled confines of West Berlin, the emblematic Cold War city often referred to as the “capital of the revolt.” Most accounts portray the events in West Berlin as having been characterized by confrontations between the leftist student movement, on the one hand, and a conservative press and generally hostile, older, urban population, on the other. This article rethinks and refines existing historiographical narratives of the 1968 student movement in West Berlin, as well as of West Berlin's place in the student movement. It examines the actions and experiences of student activists in West Berlin, who rarely feature in the familiar narrative—namely, Christian Democratic activists, particularly those from the Association of Christian Democratic Students (RCDS). Using oral history interviews, memoirs, and a wide array of archival sources from German and US archives, the article sheds light on the background of some of the most important conservative players and discusses the manifold ways in which they engaged with the goals of the revolutionary left in the city. The analysis pays special attention to the effects that German division and life in West Berlin had on Christian Democratic activists, to the sources of their anti-Communism, and to their views about the US-led war in Vietnam, a major Cold War conflict that carried special resonance in the divided city. The article concludes that there were important (yet shifting and often porous) dividing lines in West Berlin's “1968” other than those that separated politicized students from an older and more conservative city leadership and population, a conclusion that calls for a modification of the familiar storyline that simply pits Rudi Dutschke and others on the left against the city's “establishment.” The article suggests that this has repercussions for interpretations of the student movement that center on generation. It argues, in short, that Christian Democratic students—activists who were, in effect, other ’68ers—helped to shape and were, in turn, shaped by the events that took place in West Berlin in 1968.
“Crime Has No Chance”: The Discourse of Everyday Criminality in the East German Press, 1961–1989
Authors: Millington Richard 
Published: March 2017

AbstractAccording to Friedrich Engels, communists would “take an axe to the root of crime.” Criminality was, in this and similar views, “alien” to the very essence of prevailing social conditions in communist societies and ought to have disappeared as a phenomenon as soon as socialism was established. Yet, despite the ruling Socialist Unity Party's (SED) claim to have created “really existing socialism” in East Germany, crime existed and persisted. Official statistics showed that over one hundred thousand incidents of “everyday” criminal offenses, such as theft, were recorded annually. The SED regarded public relations work concerning criminality as essential to its prevention. This article examines the narrative of crime that appeared in the pages of the East German magazineNeue Berliner Illustrierte, which, following SED instructions, attempted to shape public perceptions by informing readers that crime rates were decreasing and that no serious crimes were taking place. Moreover, the articles made it clear that the only way to eliminate the causes of crime were for citizens to live according to the socialist tenets set forth by the party. As this suggests, the regime used the media and its treatment of crime and criminality in an attempt to win greater legitimacy and coopt citizens for the socialist project.
Synthetic Biology and Ethics: Past, Present, and Future
Authors: HÄYRY MATTI 
Published: March 2017

Abstract:This article explores the ethical issues that have been identified in emerging technologies, from early genetic engineering to synthetic biology. The scientific advances in the field form a continuum, and some ethical considerations can be raised time and again when new developments occur. An underlying concern is the cumulative effect of scientific advances and ensuing technological innovation that can change our understanding of life and humanity.
The Electronic Medical Record and the Loss of Narrative
Authors: MOROS DANIEL A. 
Published: March 2017

Abstract:The use of the electronic medical record (EMR) facilitates many aspects of patient care as well as clinical and outcomes research. However, our thought processes are directed differently when collecting data to be entered into a structured database compared with when collecting data to construct a narrative of the patient and his or her complaints. While recognizing that the EMR will improve overall patient care, it is worthwhile examining aspects of patient–doctor interaction that may be sacrificed.
Socioeconomic Status and Non-Fatal Adult Injuries in Selected Atlanta (Georgia USA) Hospitals
Authors: Hulland Erin , Chowdhury Ritam , Sarnat Stefanie , Chang Howard H. , Steenland Kyle 
Published: March 2017

AbstractBackgroundInjury mortality data for adults in the United States and other countries consistently show higher mortality for those with lower socioeconomic status (SES). Data are sparse regarding the role of SES among adult, non-fatal US injuries. The current study estimated non-fatal injury risk by household income using hospital emergency department (ED) visits.MethodsA total of 1,308,892 ED visits at 10 Atlanta (Georgia USA) hospitals from 2001-2004 (347,866 injuries) were studied. The SES was based on US census-block group income, with subjects assigned to census blocks based on reported residence. Logistic regression was used to determine risk by SES for injuries versus all other ED visits, adjusting for demographics, hospital, and weather. Supplemental analyses using hospital data from 2010-2013, without data on SES, were conducted to determine whether earlier patterns by race, age, and gender persisted.ResultsRisk for many injury categories increased with higher income. Odds ratio by quartiles of increasing income (lowest quartile as referent, 95% confidence interval [CI] given for upper most quartile) were 1.00, 1.23, 1.34, 1.40 (95% CI 1.36-1.45) for motor vehicle accidents; 1.00, 1.03, 1.11, 1.24 (95% CI 1.20-1.29) for being struck by objects; 1.00. 0.99, 1.04, 1.12 (95% CI 1.00-1.25) for suicide; and 1.00, 1.03, 1.05, 1.12 (95% CI 1.09-1.15) for falls. In contrast, decreased injury risk with increased household income was seen for assaults (1.00, 0.83, 0.73, 0.67 [95% CI 0.63-0.72], by increasing quartiles). These trends by income did not differ markedly by race and gender. Whites generally had less risk of injuries, with the exception of assaults and motor vehicle accidents. Males had higher risk of injury than females, with the exception of falls and suicide attempts. Patterns of risk for race, age, and gender were consistent between 2001-2004 and 2010-2013.ConclusionFor most non-fatal injuries, those with higher income had more risk of ED visits, although the opposite was true for assault.HullandE, ChowdhuryR, SarnatS, ChangHH, SteenlandK. Socioeconomic status and non-fatal adult injuries in selected Atlanta (Georgia USA) hospitals. Prehosp Disaster Med. 2017;32(4):403–413.
Do Political Science Majors Succeed in the Labor Market?
Authors: Lewis Gregory B. 
Published: March 2017

ABSTRACTDespite some stakeholders’ concerns about the practical value of an undergraduate degree in political science, our graduates actually do quite well in the labor market. Based on analysis of a sample of 3.4 million college graduates (including 86,000 in political science) from the 2009–2014 American Community Surveys, our majors earn two-thirds more than demographically similar high school graduates if they stop with bachelor’s degrees, but they are among the most likely to obtain graduate degrees, especially in law. Only engineering, economics, computer science, and health science majors make at least 10% more than our graduates, who make nearly as much as those who major in business and 10% to 25% more than those who major in most other social sciences and humanities. Political science majors have relatively high unemployment rates in their 20s, however, and may end up in very different occupations than they imagined when they chose political science.
Incentives for Sharing Knowledge: A Survey of Scholarly Practices in Public Affairs and Administration
Authors: Neely Stephen R. , Coggburn Jerrell D. 
Published: March 2017

ABSTRACTThis study examines the scholarly practice of “knowledge sharing” and the extent to which it is rewarded by prevailing faculty-incentive structures. Following recent calls for greater connectivity between the academic and practitioner communities in both political science and public administration, there is a need for greater empirical evidence regarding the extent to which these practices are being employed across the discipline and how their use varies across institutional settings. Focusing on “knowledge sharing” as a specific dimension of “engaged scholarship,” this article reports the findings from a recent survey of public affairs and administration program leaders regarding current standards for earning tenure and promotion. Relevant scholarly practices are discussed and the reported value of these practices for earning tenure and promotion is presented. Institutional types are compared and recommendations are made for improving the dissemination of scholarly knowledge to the public administration practitioner community.
Professor Favorability and Student Perceptions of Professor Ideology
Authors: Braidwood Travis , Ausderan Jacob 
Published: March 2017

ABSTRACT
Academia has become an increasingly common political target, particularly the institution of academic tenure, which many conservative politicians accuse of helping to perpetuate the ideological indoctrination of students. This study focuses on students’ perceptions of professors’ ideology by examining the link between student ideology, professor favorability, and perceptions of professors’ ideology. We employ an original survey instrument and find that, rather than forming perceptions of their professors’ political views based on their professors’ actual positions, students tend to project their own ideology onto their professor, based on the extent to which they like their professor.
Negating the Gender Citation Advantage in Political Science
Authors: Atchison Amy L. 
Published: March 2017

ABSTRACTOpen-access (OA) advocates have long promoted OA as an egalitarian alternative to traditional subscription-based academic publishing. The argument is simple: OA gives everyone access to high-quality research at no cost. In turn, this should benefit individual researchers by increasing the number of people reading and citing academic articles. As the OA movement gains traction in the academy, scholars are investing considerable research energy to determine whether there is an OA citation advantage—that is, does OA increase an article’s citation counts? Research indicates that it does. Scholars also explored patterns of gender bias in academic publishing and found that women are cited at lower rates in many disciplines. Indeed, in many disciplines, men enjoy a significant and positive gender citation effect (GCE) compared to their female colleagues. This article combines these research areas to determine whether the OA citation advantage varies by gender. Using Wilcoxon-Mann-Whitney (WMW) tests, the nonparametric analog to the independent samples T-test, I conclude that OA benefits male and female political scientists at similar rates. Thus, OA negates the gender citation advantage that typically accrues to male political scientists.
Massive star clusters in high-redshift star-forming galaxies seen at a 100 pc scale thanks to strong gravitational lensing
Authors: Dessauges-Zavadsky Miroslava , Cava Antonio , Tamburello Valentina , Schaerer Daniel , Mayer Lucio , Richard Johan , González Pablo G. Pérez 
Published: March 2017

AbstractHigh-resolution imaging reveals clumpy morphologies among z = 1 – 3 galaxies. Most of these galaxies are dominated by disk rotation, which led to conclude that the observed clumps are generated from disk fragmentation due to gravitational instability. Despite the kpc-scale resolution attained by the most advanced facilities and numerical simulations, these clumps are barely resolved at z > 1. Thanks to the stretching and magnification power provided by gravitational lensing, we reach the sub-kpc resolving power to unveil their physics. From our literature compilation of data, we show that without lensing there is a bias toward clumps with high masses and sizes. The high-redshift clumps identified in lensed galaxies have stellar masses 2 orders of magnitude lower and a median size of 250 pc. They resemble local star clusters observed in the most intensively star-forming galaxies. The clump masses and sizes observed in lensed galaxies agree with new simulations, which show that the Toomre instability criterion overestimates the clump masses by a factor of 5 – 6.
Stellar population properties of the most massive globular clusters and ultra-compact dwarf galaxies of the Fornax cluster
Authors: Hilker Michael 
Published: March 2017

AbstractMost ultra-compact dwarf galaxies (UCDs) and very massive globular clusters reside in nearby galaxy clusters or around nearby giant galaxies. Due to their distance (> 4 Mpc) and compactness (reff< 100 pc) they are barely resolved, and thus it is difficult to obtain their internal properties. Here I present our most recent attempts to constrain the mass function, stellar content and dynamical state of UCDs in the Fornax cluster. Thanks to radial velocity membership assignment of ~ 950 globular clusters (GCs) and UCDs in the core of Fornax, the shape of their mass function is well constrained. It is consistent with the ‘standard’ Gaussian mass function of GCs. Our recent simulations on the disruption process of nucleated dwarf galaxies in cluster environments showed that ~ 40% of the most massive UCDs should originate from nuclear star clusters. Some Fornax UCDs actually show evidence for this scenario, as revealed by extended low surface brightness disks around them and onsets of tidal tails. Multi-band UV to optical imaging as well as low to medium resolution spectroscopy revealed that there exist UCDs with youngish ages, (sub-)solar [α/Fe] abundances, and probably He-enriched populations.
The SUNBIRD survey: characterizing the super star cluster populations of intensely star-forming galaxies
Authors: Randriamanakoto Zara , Väisänen Petri 
Published: March 2017

AbstractSuper star clusters (SSCs) represent the youngest and most massive form of known gravitationally bound star clusters in the Universe. They are born abundantly in environments that trigger strong and violent star formation. We investigate the properties of these massive SSCs in a sample of 42 nearby starbursts and luminous infrared galaxies. The targets form the sample of the SUperNovae and starBursts in the InfraReD (SUNBIRD) survey that were imaged using near-infrared (NIR) K-band adaptive optics mounted on the Gemini/NIRI and the VLT/NaCo instruments. Results from i) the fitted power-laws to the SSC K-band luminosity functions, ii) the NIR brightest star cluster magnitude − star formation rate (SFR) relation and iii) the star cluster age and mass distributions have shown the importance of studying SSC host galaxies with high SFR levels to determine the role of the galactic environments in the star cluster formation, evolution and disruption mechanisms.
Globular clusters and the evolution of their multiple stellar populations
Authors: Chantereau W. , Charbonnel C. , Meynet G. 
Published: March 2017

AbstractOur knowledge of the formation and early evolution of globular clusters (GCs) has been totally shaken with the discovery of the peculiar chemical properties of their long-lived host stars. Therefore, the interpretation of the observed Colour Magnitude Diagrams (CMD) and of the properties of the GC stellar populations requires the use of new stellar models computed with relevant chemical compositions. In this paper we use the grid of evolution models for low-mass stars computed by Chantereau et al. (2015) with the initial compositions of second-generation stars as predicted by the fast rotating massive stars scenario to build synthesis models of GCs. We discuss the implications of the assumed initial chemical distribution on 13 Gyr isochrones. We build population synthesis models to predict the fraction of stars born with various helium abundances in present day globular clusters (assuming an age of 13 Gyr). With the current assumptions, 61 % of stars on the main sequence are predicted to be born with a helium abundance in mass fraction, Yini, smaller than 0.3 and only 11 % have a Yini larger than 0.4. Along the horizontal branch, the fraction of stars with Yini inferior to 0.3 is similar to that obtained along the main sequence band (63 %), while the fraction of very He-enriched stars is significantly decreased (only 3 % with Yini larger than 0.38).
The Imprints Of Galactic Environment On Cluster Formation and Evolution
Authors: Adamo Angela 
Published: March 2017

AbstractYoung star clusters (YSCs) appear to be a ubiquitous product of star formation in local galaxies, thus, they can be used to study the star formation process at work in their host galaxies. Moreover, YSCs are intrinsically brighter that single stars, potentially becoming the most important tracers of the recent star formation history in galaxies in the local Universe. In local galaxies, we also witness the presence of a large population of evolved star clusters, commonly called globular clusters (GCs). GCs peak formation history is very close to the redshift (z ~ 2) when the cosmic star formation history reached the maximum. Therefore, GCs are usually associated to extreme star formation episodes in high-redshift galaxies. It is yet not clear whether YSCs and GCs share a similar formation process (same physics under different interstellar medium conditions) and evolution process, and whether the former can be used as progenitor analogs of the latter. In this invited contribution, I review general properties of YSC populations in local galaxies. I will summarise some of the current open questions in the field, with particular emphasis to whether or not galactic environments, where YSCs form, leave imprints on the nested populations. The importance of this rapidly developing field can be crucial in understanding GC formation and possibly the galactic environment condition where this ancient population formed.
Environmental effects on stellar populations of star clusters and dwarf galaxies
Authors: Pasetto Stefano , Cropper Mark , Fujita Yutaka , Chiosi Cesare , Grebel Eva K. 
Published: March 2017

AbstractWe investigate the competitive role of the different dissipative phenomena acting on the onset of star formation of gravitationally bound systems in an external environment. Ram pressure, Kelvin-Helmholtz and Rayleigh-Taylor instabilities, and tidal forces are accounted for separately in an analytical framework and compared in their role in influencing the star forming regions. We present an analytical criterion to elucidate the dependence of star formation in a spherical stellar system on its surrounding environment. We consider the different signatures of these phenomena in synthetically realized colour-magnitude diagrams (CMDs) of the orbiting system thus investigating the detectability limits of these different effects for future observational projects and their relevance. The developed theoretical framework has direct applications to the cases of massive star clusters, dwarf galaxies in galaxy clusters and dwarf galaxies orbiting our Milky Way system, as well as any primordial gas-rich cluster of stars orbiting within its host galaxy.
Massive cold cloud clusters
Authors: Toth L. Viktor , Zahorecz Sarolta , Marton Gabor , Ristorcelli Isabelle , Juvela Mika , Montier Ludovic , Bernard Jean-Philippe 
Published: March 2017

AbstractThe all-sky Planck catalogue of Galactic Cold Clumps (PGCC) allows an almost unbiased study of the early phases of star-formation in our Galaxy. Several thousand of the clumps have also distance estimates allowing a determination of mass and density. The nature of Planck cold clumps varies from IRDCs to tiny nearby cold clouds with masses ranging from one to several tens of thousands solar masses. Some of the clumps are embedded in GMCs, others are isolated. Some are close or even very close to OB associations, while others lay far from any UV luminous objects. The small scale clustering of nearby PGCCs was studied with the improved Minimum Spanning Tree (MST) method identifying groups in 3D space, locating also massive cold cloud clusters eg. PGCCMST G210.6-19.5 in LDN 1641.
Are Galactic globular cluster AGB stars rich or poor in Sodium? Sodium abundance of AGB and RGB stars in NGC 2808
Authors: Wang Yue , Primas Francesca , Charbonnel Corinne , Van der Swaelmen Mathieu , Chantereau William , Bono Giuseppe 
Published: March 2017

AbstractA spectroscopic study comparing the [Na/Fe] distributions of RGB and AGB stars in the Galactic globular cluster (GC) NGC 6752 found that there was no Na-rich, 2nd-generation star along the early-AGB of this cluster. This came as a surprise since in this GC, as well as other Galactic GCs studied so far, 1st- and 2nd-generation stars have usually been found from the main sequence turnoff up to the red giant branch. To investigate whether the failure of a significant fraction of stars to ascend the AGB also happens to other GCs, we studied a sample of AGB and RGB stars in NGC 2808 observed at the ESO/VLT with FLAMES. Contrary to NGC 6752, we find that the AGB and RGB stars we studied in NGC 2808 have comparable [Na/Fe] dispersions.
Dissecting 30 Doradus: Optical and Near Infrared Star Formation History of the starburst cluster NGC2070 from the Hubble Tarantula Treasury Project
Authors: Cignoni Michele ,   the HTTP team
Published: March 2017

AbstractI will present new results on the star formation history of 30 Doradus in the Large Magellanic Cloud based on the panchromatic imaging survey Hubble Tarantula Treasury Project (HTTP). Here the focus is on the starburst cluster NGC2070. The star formation history is derived by comparing the deepest ever optical and NIR color-magnitude diagrams (CMDs) with state-of-the-art synthetic CMDs generated with the latest PARSEC models, which include all stellar phases from pre-main sequence to post-main sequence. For the first time in this region we are able to measure the star formation using intermediate and low mass stars simultaneously. Our results suggest that NGC2070 experienced a prolonged activity. I will discuss the detailed star formation history, initial mass function and reddening distribution.
Mid-infrared [NeII] Imaging of Young Massive Star Clusters Near Galactic Nuclei
Authors: Yeh Sherry C. C. , Tsai Chao-Wei , Geballe Thomas R. , Herrera Cinthya N. 
Published: March 2017

AbstractWe investigate the formation of young massive clusters near the nuclei in NGC 6946, IC 342, Maffei II, and NGC 7714, using ground-based mid-infrared [NeII] imaging. We derive the cluster formation efficiency and cluster mass function, and the results suggest that environmental effects on YMC formation may not be significant.