bluuebunny/crossref_metadata_2025_split huggingface dataset:
Práticas Pedagógicas Inclusivas: Análise das Salas de Recursos Multifuncionais em Curitiba
Authors: Silva Lourival Claudino da 
Published: December 2024

Introdução: Este estudo investigou a dinâmica da Educação Especial Inclusiva no âmbito da legislação educacional brasileira e no contexto das Salas de Recursos Multifuncionais no estado do Paraná, destacando a importância de promover a inclusão para garantir o desenvolvimento pleno de todos os discentes. Objetivo: O problema identificado foi a falta de formação adequada dos professores que atuam nas Salas de Recursos Multifuncionais, resultando em desafios na prestação de um atendimento de qualidade. O objetivo geral foi compreender o contexto da educação inclusiva e analisar a formação de professores, além de investigar práticas inclusivas nessas salas. Método: Utilizou-se uma pesquisa bibliográfica de caráter descritivo e exploratório, com a análise da legislação e normativas educacionais vigentes no Brasil. A pesquisa de campo consistiu em um levantamento por meio de questionários realizados em oito escolas no bairro Cajuru, em Curitiba, abrangendo as ações realizadas nos anos de 2022 e 2023. Resultados: Foram identificados desafios específicos, como a avaliação contínua pela equipe da sala, a acessibilidade do ambiente, o envolvimento dos pais e a frequência dos alunos. Os dados coletados evidenciaram a importância da formação continuada dos professores e a necessidade de um profissional capacitado para a gestão das Salas de Recursos Multifuncionais. Conclusões: As considerações finais indicaram que a formação adequada dos educadores é essencial para garantir um atendimento de qualidade e promover práticas pedagógicas inclusivas. Destacou-se a importância do "recurso humano" no Atendimento Educacional Especializado, enfatizando que a negligência nesse aspecto pode comprometer a missão da escola em sua função de ensino-aprendizagem. Foi sugerida a necessidade de estudos futuros para explorar melhores práticas na formação de professores e na gestão das Salas de Recursos Multifuncionais, contribuindo para um ambiente educacional mais inclusivo e igualitário.
Towards a communication strategy implementation framework for higher education institutions in Lesotho
Authors: Letlatsa Relebohile 
Published: December 2024

This article reports on the findings of a research study of three Higher Education Institutions (HEI) in Lesotho on the communication strategies they use to engage with internal and external stakeholders to implement their institutional strategies. A mixed-method research approach was followed, and a sample of three HEIs and their internal and external stakeholders was identified through a multidimensional sampling strategy. Triangulation included a survey among stakeholders, interviews with senior managers, and a content analysis of strategic plans. Statistical analysis was conducted on quantitative data, thematic analysis on qualitative data from interviews and open-ended survey items, and content analysis on strategic plans. Leximancer software was used for the qualitative data analysis. Results indicate the importance for the institutions to develop communication strategies; align institutional strategies with organisational culture; identify legitimate and strategic stakeholders; and use fitting communication platforms to disseminate information to all stakeholders.
Effects of Background Solar Wind and Drag Force on the Propagation of Coronal-mass-ejection-driven Shocks
Authors: Wu Chin-Chun , Liou Kan , Wood Brian E. , Hutting Lynn 
Published: December 2024

Abstract
The propagation of interplanetary shocks, particularly those driven by coronal mass ejections (CMEs), is still an outstanding question in heliophysics and space weather forecasting. Here, we address the effects of the ambient solar wind on the propagation of two similar CME-driven shocks from the Sun to Earth. The two shock events (CME03, 2010 April 3; CME12, 2012 July 12) have the following properties. Both events (1) were driven by a halo CME (i.e., the source location is near the Sun–Earth line); (2) had a CME source in the southern hemisphere; (3) had a similar transit time (∼2 days) to Earth; (4) occurred in a nonquiet solar period; and (5) led to a severe geomagnetic storm. The initial (near the Sun) propagation speed, as measured by coronagraph images, was slower (by ∼300 km s−1) for CME03 than CME12, but it took about the same amount of traveling time for both events to reach Earth. According to the in situ solar wind observations from the Wind spacecraft, the CME03-driven shock was associated with a faster solar wind upstream of the shock than the CME12-driven shock. This is also demonstrated in our global MHD simulations. Analysis of our simulation result indicates that the drag force indirectly plays an important role in the shock propagation. The present study suggests that in addition to the initial CME propagation speed near the Sun, the shock speed (in the inertial frame) and the ambient solar wind conditions—in particular, the solar wind speed—are key to timing the arrival of CME-driven shock events.
Do Neutron Star Ultraluminous X-Ray Sources Masquerade as Intermediate-mass Black Holes in Radio and X-Ray?
Authors: Panurach Teresa , Dage Kristen C. , Urquhart Ryan , Plotkin Richard M. , Paul Jeremiah D. , Bahramian Arash , Brumback McKinley C. , Galvin Timothy J. , Molina Isabella , Miller-Jones James C. A. , Saikia Payaswini 
Published: December 2024

Abstract
Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve as potential candidates for (sub-Eddington) intermediate-mass black holes. However, a total of eight ULXs have now been confirmed to be powered by neutron stars, thanks to observed pulsations, and may act as contaminants for the radio/X-ray selection of intermediate-mass black holes. Here, we present the first comprehensive radio study of seven known neutron star ULXs using new and archival data from the Karl G. Jansky Very Large Array and the Australia Telescope Compact Array, combined with the literature. Across this sample, there is only one confident radio detection, from the Galactic neutron star ULX Swift J0243.6+6124. The other six objects in our sample are extragalactic, and only one has coincident radio emission, which we conclude is most likely contamination from a background H ii region. We conclude that with current facilities, neutron star ULXs do not produce significant enough radio emission to cause them to be misidentified as radio-/X-ray-selected intermediate-mass black hole candidates. Thus, if background star formation has been properly considered, the current study indicates that a ULX with a compact radio counterpart is not likely to be a neutron star.
Exact Nonlinear Decomposition of Ideal-MHD Waves Using Eigenenergies. II. Fully Analytical Equations and Pseudoadvective Eigenenergies
Authors: Raboonik Abbas , Pontin David I. , Tarr Lucas A. 
Published: December 2024

Abstract
Physical insight into plasma evolution in the magnetohydrodynamic (MHD) limit can be revealed by decomposing the evolution according to the characteristic modes of the system. In this paper we explore aspects of the eigenenergy decomposition method (EEDM) introduced in an earlier study (ApJ, 967:80). The EEDM provides an exact decomposition of nonlinear MHD disturbances into their component eigenenergies associated with the slow, Alfvén, and fast eigenmodes, together with two zero-frequency eigenmodes. Here we refine the EEDM by presenting globally analytical expressions for the eigenenergies. We also explore the nature of the zero-frequency “pseudoadvective (PA) modes” in detail. We show that in evolutions with pure advection of magnetic and thermal energy (without propagating waves), a part of the energy is carried by the PA modes. Exact expressions for the error terms associated with these modes—commonly encountered in numerical simulations—are also introduced. The new EEDM equations provide a robust tool for the exact and unique decomposition of nonlinear disturbances governed by homogeneous quasi-linear partial differential equations, even in the presence of local or global degeneracies.
Modeling the Multiwavelength Detection of Protoclusters. I. An Excess of Submillimeter Galaxies in Protocluster Cores
Authors: Araya-Araya Pablo , Cochrane Rachel K. , Hayward Christopher C. , Yates Robert M. , Sodré Laerte , Vicentin Marcelo C. , Rennehan Douglas , Overzier Roderik , van Daalen Marcel 
Published: December 2024

Abstract
Studies of galaxy protoclusters yield insights into galaxy cluster formation complementary to those obtained via “archaeological” studies of present-day galaxy clusters. Submillimeter-selected galaxies (SMGs) are one class of sources used to find high-redshift protoclusters. However, due to the rarity of protoclusters (and thus the large simulation volume required) and the complexity of modeling dust emission from galaxies, the relationship between SMGs and protoclusters has not been adequately addressed in the theoretical literature. In this work, we apply the L-GALAXIES semianalytic model (SAM) to the Millennium
N-body simulation. We assign submillimeter flux densities to the model galaxies using a scaling relation from previous work, in which dust radiative transfer was performed on high-resolution galaxy zoom simulations. We find that the fraction of model galaxies that are submillimeter-bright is higher in protocluster cores than in both protocluster “outskirts” and the field; the fractions for the latter two are similar. This excess is not driven by an enhanced starburst frequency. Instead, the primary reason is that overdense environments have a relative overdensity of high-mass halos and thus “oversample” the high-mass end of the star formation main sequence relative to less-dense environments. The fraction of SMGs that are optically bright is dependent on stellar mass and redshift but independent of the environment. The fraction of galaxies for which the majority of star formation is dust-obscured is higher in protocluster cores, primarily due to the dust-obscured fraction being correlated with stellar mass. Our results can be used to guide and interpret multiwavelength studies of galaxy populations in protoclusters.
Millinovae: A New Class of Transient Supersoft X-Ray Sources without a Classical Nova Eruption
Authors: Mróz Przemek , Król Krzysztof , Szegedi Hélène , Charles Philip , Page Kim L. , Udalski Andrzej , Buckley David A. H. , Dewangan Gulab , Meintjes Pieter , Szymański Michał K. , Soszyński Igor , Pietrukowicz Paweł , Kozłowski Szymon , Poleski Radosław , Skowron Jan , Ulaczyk Krzysztof , Gromadzki Mariusz , Rybicki Krzysztof , Iwanek Patryk , Wrona Marcin , Mróz Mateusz J. 
Published: December 2024

Abstract
Some accreting binary systems containing a white dwarf (such as classical novae or persistent supersoft sources) are seen to emit low-energy X-rays with temperatures of ∼ 106 K and luminosities exceeding 1035 erg s−1. These X-rays are thought to originate from nuclear burning on the white dwarf surface, either caused by a thermonuclear runaway (classical novae) or a high mass-accretion rate that sustains steady nuclear burning (persistent sources). The discovery of transient supersoft X-rays from ASASSN-16oh challenged these ideas, as no clear signatures of mass ejection indicative of a classical nova eruption were detected, and the origin of these X-rays remains controversial. It was unclear whether this star was one of a kind or representative of a larger, as yet undiscovered, group. Here, we present the discovery of 29 stars located in the direction of the Magellanic Clouds exhibiting long-duration, symmetrical optical outbursts similar to that seen in ASASSN-16oh. We observed one of these objects during an optical outburst and found it to be emitting transient supersoft X-rays, while no signatures of mass ejection (indicative of a classical nova eruption) were detected. We therefore propose that these objects form a homogeneous group of transient supersoft X-ray sources, which we dub “millinovae” because their optical luminosities are approximately a 1000 times fainter than those of ordinary classical novae.
Robust Detection of Hot Intragroup Medium in Optically Selected, Poor Galaxy Groups by eROSITA
Authors: Li Dawei , Fang Taotao , Ge Chong , Liu Teng , He Lin , Li Zhiyuan , Nicastro Fabrizio , Yang Xiaohu , Zhang Xiaoxia , Zheng Yun-Liang 
Published: December 2024

Abstract
Over the last several decades, extensive research has been conducted on the baryon cycles within cosmic structures, encompassing a broad mass range from dwarf galaxies to galaxy clusters. However, a notable gap in understanding the cosmic baryon cycle is the poor galaxy groups with halo masses around 1013
M
⊙. Poor galaxy groups, like our own Local Group, are prevalent throughout the Universe, yet robust detection of their hot, X-ray-emitting intragroup medium (IGrM) has remained elusive. The presence of this hot IGrM is crucial for addressing the long-standing “missing baryons” problem. Previous ROSAT-based studies were limited by a small number of X-ray bright samples, thus restricting the scope of their findings. Here, we show a robust detection of this hot IGrM in a large, optically selected poor groups sample, based on the stacked X-ray images from the eROSITA Final Equatorial Depth Survey. These groups are identified in DESI Legacy Survey with a mass range of log(M
halo/h
−1
M
⊙) = 11.5–13.5 and a redshift range of z = 0.1–0.5. Additionally, our results indicate that despite its presence in virtually groups at all sizes, this gas component is still not sufficient to recover the universal baryon fraction, and hence the “missing baryons” problem still persists in poor galaxy groups.
Hinaus in die Ferne! Lebensreform et randonnée
Authors: Milon Claire 
Published: December 2024

La randonnée se développe à la fin du xixe siècle en Allemagne et entretient une certaine proximité avec les mouvements de la Lebensreform, comme pratique du corps et pratique de nature. En tant qu’activité de plein air, la randonnée est par nature spatialisée. Elle est un mouvement de fuite hors des villes, qui met en relation l’espace urbain, dessiné en négatif, et les espaces perçus comme « naturels », territoires d’explorations corporelle et intérieure. Au fondement même de la randonnée, l’itinérance suppose l’acquisition de compétences spatiales et techniques particulières. La randonnée est un mouvement de la Lebensreform au sein duquel se joue un double rapport avec l’espace : l’activité n’a de sens que par les territoires traversés, mais ces lieux sont dans le même temps transformés par la présence des randonneuses et randonneurs.
Challenges in status disclosure and adherence to antiretroviral therapy in children living with HIV: An observational study
Authors: Aggarwal Shivali , Walia Rupinder , Chopra Dimple , Malhotra Vishal , Gupta Sharang , Malhan Shreya , Singh Harmeet 
Published: December 2024

Background and Objectives:
The advent of highly active antiretroviral therapy has increased the longevity in children living with HIV (CLHIV), which has brought forth new concerns related to status disclosure and adherence to treatment. Information regarding this is limited in Punjab; hence, this study was done to find the relation of disclosure with sociodemographic factors and the problems faced in adhering to antiretroviral therapy (ART) in this region.

Materials and Methods:
An observational cross-sectional study was conducted on CLHIVs aged 18 months to 15 years visiting the ART center of a tertiary hospital from June to December 2021. Willing caregivers were approached with semistructured validated pretested questionnaire developed for the study.

Results:
Ninety-eight caregivers of CLHIV were interviewed and 25% were found to be aware of their serostatus. Children between 5 and 12 years comprised the largest group (57%) and this was also the statistically significant age group in whom the status was not disclosed. Disclosure was more in children having single parents. The low economic status, rural background, and low education status of the caregivers were inversely related to disclosure. Sixty-five percent of the caregivers believed that the appropriate age for status disclosure should be 14–18 years. Adherence was optimal in 85% CLHIVs and distance was the foremost challenge.

Conclusion:
The mean age for disclosure was found to be higher than the World Health Organization guidelines in this study; hence, there is a need to encourage caregivers for timely and systematic disclosure and motivate them for maintaining optimal adherence in CLHIV which is important for the success of ART program.
A unique case of humungous metastasis of follicular carcinoma in the gluteal region
Authors: Priyanka D. V. S. , Raju Kalyani , Suresh T. N. , Shilpa M. D. 
Published: December 2024

ABSTRACT
Follicular thyroid carcinoma is a notable subtype of thyroid carcinoma, with metastasis accounting for 6%–20% of cases and typically characterised by haematogenous spread to the lung, liver and bone. We are reporting a rare case in which a 67-year-old male presented with swelling over his left gluteal region. On local examination, a hard mass on the left side of the gluteal region was discovered, which radiologically was determined to be chondrosarcoma/soft-tissue sarcoma. Cytology revealed metastatic deposits of adenocarcinoma. Histopathological examination revealed follicular carcinoma metastasis.
A Brief History of Traditional Indian Medicine: In Particular, Yoga and Siddha Systems of Medicine; Part 2 – Evidence-based Ancient History of India that is Bharat, Revisited
Authors: Seshadri Hiramalini , Seshadri Divya 
Published: December 2024

Abstract
A brief history of traditional Indian medicine, in particular, Yoga and Siddha systems of medicine, is presented as a four-part series including Part 1 – Why Indian medicos need to know of the rich medical heritage of Bharat, an eye-opener, Part 2 – Evidence-based ancient history of India that is Bharat, revisited, Part 3 – A brief on the knowledge level of ancient India and knowledge codified under Yoga, pertaining to optimum health and maximising human potential and Part 4 – A brief on the Siddha system of medicine, including their knowledge level and the Siddha contribution to medical education in the ancient world. India’s rich medical heritage has been kept away from India and the world in general by a distorted colonial narrative. In this second part of the series, why we need to revisit the history of ancient India is discussed; evidence that suggests that an advanced civilisation existed in peninsular India in pre-historic times, which went under ocean waters due to sea level rise, is presented; and emerging evidence available on the history of traditional Indian medicine, mainly Siddha medicine which belongs to those timelines, is presented.
Estimation of Air Travel–Related Greenhouse Gas Emissions for the In-Person Anesthesiology Oral Board Examination
Authors: Clegg Alan , Mastrantonio Sierra , Pearson John F. 
Published: December 2024

Background With an increased focus on climate change in graduate medical education (GME), the environmental implications of travel for board certification examinations remain poorly described. The return to the mandatory in-person applied examination (AE) for board eligible anesthesiologists presents potentially sizeable greenhouse gas (GHG) emissions when compared to the virtual format administered during the COVID-19 pandemic.
Objective To estimate the GHG emissions from air travel to the in-person AE and discuss its implications for various specialties as they return to in-person examinations.
Methods An estimate of the GHG emissions was conducted using data from the 2023 NRMP Main Residency Match: Match Rates by Specialty and State report, utilizing residency training site as a proxy for anesthesiologists’ home. An alternative estimate was made using the anesthesiologists’ predicted state distribution postgraduation. We estimated annual GHG emissions, expressed as metric tons of carbon dioxide equivalent (MTCO2e), produced from graduating residents flying to The American Board of Anesthesiology testing center in Raleigh, North Carolina, USA. We collected emissions using the International Civil Aviation Organization emissions calculator.
Results Annual emissions of examinee travel from their respective residency training state was estimated to be 517.37 MTCO2e. The alternative estimate using anesthesiologists’ predicted postgraduation state was 568.05 MTCO2e. This estimate of CO2e roughly equates to the average annual emissions produced by 112 passenger vehicles.
Conclusions The AE in-person format results in an estimated 517 to 568 MTCO2e.
International Planetary Health Education in Undergraduate and Graduate Medical Curricula: A Scoping Review
Authors: Selvam Rajajee , Séguin Niève , Zhang Lisa , Lacaille-Ranger Ariane , Sikora Lindsey , Raiche Isabelle , McIsaac Daniel I. , Moloo Husein 
Published: December 2024

Background Climate change is a public health emergency, yet planetary health education is absent for many medical and health professions trainees.
Objective To perform a scoping review exploring the inclusion of planetary health in undergraduate and graduate medical education.
Methods A search strategy was developed with a health sciences librarian and run on 6 databases from their inception to February 2022: MEDLINE, Embase, APA PsycInfo, CINAHL, Global Health, and Scopus. The Arksey and O’Malley framework was employed to broadly select publications that described the implementation of planetary health in undergraduate and postgraduate medical education. Commentaries were included if they outlined a potential curriculum. Extracted data was grouped thematically using an iterative approach based on competencies described, key considerations, and anticipated barriers.
Results After screening 2407 articles, 42 were included. Thirty articles involved medical education at undergraduate or postgraduate levels, while 10 discussed multidisciplinary education including veterinary medicine, public health, and nursing. Two articles discussed planetary heath education for staff physicians. Reported competencies included eco-medical literacy, environmental inequity, and planetary health advocacy. Key considerations for curricular development included longitudinal implementation, interprofessional collaboration, and experiential learning through quality improvement projects. Barriers to implementation included time constraints and the lack of knowledgeable educators and administrative support for curricular change.
Conclusions This scoping review outlines key recommendations and barriers to help facilitate the implementation of planetary health education in medical training.