Evolving supernova remnants in multiphase interstellar media

We performed three-dimensional magnetohydrodynamic simulations to study the evolution of a supernova remnant (SNR) in a turbulent neutral atomic interstellar medium. The media used as background shares characteristics with the Solar neighbourhood and the SNR has mass and energy similar to those of a Type Ia object. Our initial conditions consist of dense clouds in a diluted medium, with the main difference between simulations being the average magnitude of the magnetic field. We measured amplifications of the magnetic energy of up to 34 per cent, and we generated synthetic maps that illustrate how the same object can show different apparent geometries and physical properties when observed through different lines of sight.Fil: Villagran Azuara, Marco Adrian. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Velazquez, Paula Florencia. Universidad Nacional Autónoma de México; MéxicoFil: Gomez, Daniel Osvaldo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; ArgentinaFil: Giacani, Elsa Beatriz. Universidad de Buenos Aires. Facultad de Arquitectura, Diseño y Urbanismo; Argentina. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentin

A blowout numerical model for the supernova remnant G352.7-0.1

We present 3D hydrodynamical simulations of the Galactic supernova remnant G352.7−0.1. This remnant is peculiar for having a shell-like inner ring structure and an outer arc in radio observations. In our model, the supernova explosion producing the remnant occurs inside and near the border of a spherical cloud with a density higher than that of the surrounding interstellar medium. A blowout is produced when the remnant reaches the border of the cloud. We have then used the results of our hydrodynamical simulations to calculate synthetic synchrotron radio emission maps, as well as synthetic X-ray maps. For some combinations of the particle acceleration mechanism and the direction of the line of sight, our radio maps display the peculiar morphology of G352.7−0.1 and reproduce the correct relative sizes of the main observed features. At the same time, the calculated X-ray maps reproduce the centrally peaked morphology of the observations.Fil: Toledo Roy, J. C.. Universidad Nacional Autónoma de México; MéxicoFil: Velazquez, P. F.. Universidad Nacional Autónoma de México; MéxicoFil: Esquivel, A.. Universidad Nacional Autónoma de México; MéxicoFil: Giacani, Elsa Beatriz. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentin

Origin of the bilateral structure of the supernova remnant G296.5+10

In this work, we have modelled the supernova remnant (SNR) G296.5+10, by means of 3D magnetohydrodynamics (MHD) simulations. This remnant belongs to the bilateral SNR group and has an additional striking feature: the rotation measure (RM) in its eastern and western parts are very different. In order to explain both the morphology observed in radio-continuum and the RM, we consider that the remnant expands into a medium shaped by the superposition of the magnetic field of the progenitor star with a constant Galactic magnetic field. We have also carried out a polarization study from our MHD results, obtaining synthetic maps of the linearly polarized intensity and the Stokes parameters. This study reveals that both the radio morphology and the reported RM for G296.5+10 can be explained if the quasi-parallel acceleration mechanism is taking place in the shock front of this remnant.Fil: Moranchel-Basurto, A.. Universidad Nacional Autónoma de México; MéxicoFil: Velazquez, P.. Universidad Nacional Autónoma de México; MéxicoFil: Giacani, Elsa Beatriz. Universidad de Buenos Aires. Facultad de Arquitectura y Urbanismo; Argentina. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Toledo Roy, J. C.. Universidad Nacional Autónoma de México; MéxicoFil: Schneiter, E.. Universidad Nacional Autónoma de México; MéxicoFil: De Colle, F.. Universidad Nacional Autónoma de México; MéxicoFil: Esquivel, A.. Universidad Nacional Autónoma de México; Méxic

Analytical Performance of a Multiplex Real-Time PCR Assay Using TaqMan Probes for Quantification of Trypanosoma cruzi Satellite DNA in Blood Samples

Background: The analytical validation of sensitive, accurate and standardized Real-Time PCR methods for Trypanosoma cruzi quantification is crucial to provide a reliable laboratory tool for diagnosis of recent infections as well as for monitoring treatment efficacy. Methods/Principal Findings: We have standardized and validated a multiplex Real-Time quantitative PCR assay (qPCR) based on TaqMan technology, aiming to quantify T. cruzi satellite DNA as well as an internal amplification control (IAC) in a single-tube reaction. IAC amplification allows rule out false negative PCR results due to inhibitory substances or loss of DNA during sample processing. The assay has a limit of detection (LOD) of 0.70 parasite equivalents/mL and a limit of quantification (LOQ) of 1.53 parasite equivalents/mL starting from non-boiled Guanidine EDTA blood spiked with T. cruzi CLBrener stock. The method was evaluated with blood samples collected from Chagas disease patients experiencing different clinical stages and epidemiological scenarios: 1- Sixteen Venezuelan patients from an outbreak of oral transmission, 2- Sixty three Bolivian patients suffering chronic Chagas disease, 3- Thirty four Argentinean cases with chronic Chagas disease, 4- Twenty seven newborns to seropositive mothers, 5- A seronegative receptor who got infected after transplantation with a cadaveric kidney explanted from an infected subject. Conclusions/Significance: The performing parameters of this assay encourage its application to early assessment of T. cruzi infection in cases in which serological methods are not informative, such as recent infections by oral contamination or congenital transmission or after transplantation with organs from seropositive donors, as well as for monitoring Chagas disease patients under etiological treatment.Fil: Duffy, Tomas. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Investigaciones En Ingeniería Genética y Biología Molecular; ArgentinaFil: Cura, Carolina Inés. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Investigaciones en Ingeniería Genética y Biología Molecular; ArgentinaFil: Ramírez, Juan C.. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Investigaciones en Ingeniería Genética y Biología Molecular; ArgentinaFil: Abate, Teresa. Universidad Central de Venezuela. Instituto de Medicina Tropical; VenezuelaFil: Cayo, Nelly M.. Universidad Nacional de Jujuy. Instituto de Biologia de la Altura; ArgentinaFil: Parrado, Rudy. Universidad San Simón; BoliviaFil: Diaz Bello, Zoraida. Universidad Central de Venezuela. Instituto de Medicina Tropical; VenezuelaFil: Velazquez, Elsa Beatriz. Dirección Nacional de Instituto de Investigación. Administración Nacional de Laboratorio e Instituto de Salud. Instituto Nacional de Parasitología; ArgentinaFil: Muñoz Calderón, Arturo. Universidad Central de Venezuela. Instituto de Medicina Tropical; VenezuelaFil: Juiz, Natalia Anahí. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Investigaciones en Ingeniería Genética y Biología Molecular; ArgentinaFil: Basile, Joaquín. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Investigaciones en Ingeniería Genética y Biología Molecular; ArgentinaFil: Garcia, Lineth. Universidad San Simón; BoliviaFil: Riarte, Adelina. Dirección Nacional de Instituto de Investigación. Administración Nacional de Laboratorio e Instituto de Salud. Instituto Nacional de Parasitología; ArgentinaFil: Nasser, Julio Rubén. Universidad Nacional de Salta. Facultad de Ciencias Naturales; ArgentinaFil: Ocampo, Susana B.. Universidad Nacional de Jujuy. Instituto de Biologia de la Altura; ArgentinaFil: Yadon, Zaida E.. Pan-American Health Organization; Estados UnidosFil: Torrico, Faustino. Universidad San Simón; BoliviaFil: Alarcón de Noya, Belkisyole. Universidad Central de Venezuela. Instituto de Medicina Tropical; VenezuelaFil: Ribeiro, Isabela. Drugs and Neglected Diseases Initiative; SuizaFil: Schijman, Alejandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Investigaciones en Ingeniería Genética y Biología Molecular; Argentin

Effects of thermal conduction on the X-ray and synchrotron emission from supernova remnants

Several physical mechanisms have been studied in order to explain why composite supernova remnants (SNRs) have shell-like morphologies in the radio continuum while their X-ray emission is centrally peaked. One of the proposed mechanisms has been the presence of thermal conduction, which can raise the density at the center of SNRs, increasing the X-ray emission from these regions. In this work, we have carried out axisymmetric numerical simulations with the adaptive grid Yguazú-a code, which includes advection of the magnetic field and thermal conduction. We have considered cases with anisotropic and isotropic thermal conduction, as well as with no conduction. We have simulated X-ray (as well as radio synchrotron) emission maps from our numerical simulations, which can be directly compared with observations.Fil: Velazquez, Pablo F.. Universidad Nacional Autónoma de México; MéxicoFil: Martinell, Julio J.. Universidad Nacional Autónoma de México; MéxicoFil: Raga, Alejandro C.. Universidad Nacional Autónoma de México; MéxicoFil: Giacani, Elsa Beatriz. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentin

Socioeconomic, Clinical, and Molecular Features of Breast Cancer Influence Overall Survival of Latin American Women

Molecular profile of breast cancer in Latin-American women was studied in five countries: Argentina, Brazil, Chile, Mexico, and Uruguay. Data about socioeconomic characteristics, risk factors, prognostic factors, and molecular subtypes were described, and the 60-month overall cumulative survival probabilities (OS) were estimated. From 2011 to 2013, 1,300 eligible Latin-American women 18 years or older, with a diagnosis of breast cancer in clinical stage II or III, and performance status ≦̸1 were invited to participate in a prospective cohort study. Face-to-face interviews were conducted, and clinical and outcome data, including death, were extracted from medical records. Unadjusted associations were evaluated by Chi-squared and Fisher’s exact tests and the OS by Kaplan–Meier method. Log-rank test was used to determine differences between cumulative probability curves. Multivariable adjustment was carried out by entering potential confounders in the Cox regression model. The OS at 60 months was 83.9%. Multivariable-adjusted death hazard differences were found for women living in Argentina (2.27), Chile (1.95), and Uruguay (2.42) compared with Mexican women, for older (≥60 years) (1.84) compared with younger (≤40 years) women, for basal-like subtype (5.8), luminal B (2.43), and HER2-enriched (2.52) compared with luminal A subtype, and for tumor clinical stages IIB (1.91), IIIA (3.54), and IIIB (3.94) compared with stage IIA women. OS was associated with country of residence, PAM50 intrinsic subtype, age, and tumor stage at diagnosis. While the latter is known to be influenced by access to care, including cancer screening, timely diagnosis and treatment, including access to more effective treatment protocols, it may also influence epigenetic changes that, potentially, impact molecular subtypes. Data derived from heretofore understudied populations with unique geographic ancestry and sociocultural experiences are critical to furthering our understanding of this complexity. Copyright © 2022 de Almeida, Cortés, Vilensky, Valenzuela, Cortes-Sanabria, de Souza, Barbeito, Abdelhay, Artagaveytia, Daneri-Navarro, Llera, Müller, Podhajcer, Velazquez, Alcoba, Alonso, Bravo, Camejo, Carraro, Castro, Cataldi, Cayota, Cerda, Colombo, Crocamo, Del Toro-Arreola, Delgadillo-Cristerna, Delgado, Breitenbach, Fernández, Fernández, Fernández, Franco-Topete, Gaete, Gómez, Gonzalez-Ramirez, Guerrero, Gutierrez-Rubio, Jalfin, Lopez-Vazquez, Loria, Míguez, Moran-Mendoza, Morgan-Villela, Mussetti, Nagai, Oceguera-Villanueva, Reis, Retamales, Rodriguez, Rosales, Salas-Gonzalez, Segovia, Sendoya, Silva-Garcia, Viña, Zagame, Jones, Szklo and United States-Latin American Cancer Research Network (US-LACRN).Fil: de Almeida, Liz Maria. Instituto Nacional de Cáncer; BrasilFil: Cortés, Sandra. Pontificia Universidad Católica de Chile; ChileFil: Vilensky, Marta. Instituto de Oncología Angel Roffo; ArgentinaFil: Valenzuela, Olivia. Universidad de Sonora; MéxicoFil: Cortes-Sanabria, Laura. Hospital de Especialidades, CMNO-IMSS; MéxicoFil: de Souza, Mirian. Instituto Nacional de Cáncer; BrasilFil: Barbeito, Rafael Alonso. Facultad de Medicina; ArgentinaFil: Abdelhay, Eliana. Instituto Nacional de Cáncer; BrasilFil: Artagaveytia, Nora. Hospital de Clínicas Manuel Quintela. Universidad de la República; UruguayFil: Daneri-Navarro, Adrian. Universidad de Guadalajara; MéxicoFil: Llera, Andrea S. CONICET. Fundación Instituto Leloir; ArgentinaFil: Müller, Bettina. Instituto Nacional del Cáncer; ArgentinaFil: Podhajcer, Osvaldo L. CONICET. Fundación Instituto Leloir; ArgentinaFil: Velazquez, Carlos. Universidad de Sonora; MéxicoFil: Alcoba, Elsa. Hospital Municipal de Oncología María Curie; ArgentinaFil: Alonso, Isabel. Centro Hospitalario Pereira Rossell; ArgentinaFil: Bravo, Alicia I. Hospital Regional de Agudos Eva Perón; ArgentinaFil: Camejo, Natalia. Hospital de Clínicas Manuel Quintela. Universidad de la República; UruguayFil: Carraro, Dirce Maria. AC Camargo Cancer Center; BrasilFil: Castro, Mónica. Instituto de Oncología Angel Roffo; ArgentinaFil: Cataldi, Sandra. Instituto Nacional de Cáncer; UruguayFil: Cayota, Alfonso. Institut Pasteur de Montevideo; UruguayFil: Cerda, Mauricio. Universidad de Chile; ChileFil: Colombo, Alicia. Universidad de Chile; ChileFil: Crocamo, Susanne. Instituto Nacional de Cáncer; BrasilFil: Del Toro-Arreola, Alicia. Universidad de Guadalajara; MéxicoFil: Delgadillo-Cristerna, Raul. Hospital de Especialidades. CMNO-IMSS; MéxicoFil: Delgado, Lucia. Hospital de Clínicas Manuel Quintela; UruguayFil: Breitenbach, Marisa Dreyer. Universidade do Estado do Rio de Janeiro; BrasilFil: Fernández, Elmer. Universidad Católica de Córdoba. CONICET. Centro de Investigaciones en Bioquímica Clínica e Inmunologia; ArgentinaFil: Fernández, Jorge. Instituto de Salud Pública; ChileFil: Fernández, Wanda. Hospital San Borja Arriarán; ChileFil: Franco-Topete, Ramon A. OPD Hospital Civil de Guadalajara. Universidad de Guadalajara; MéxicoFil: Gaete, Fancy. Hospital Luis Tisne; ChileFil: Gómez, Jorge. Texas A&M University; Estados UnidosFil: Gonzalez-Ramirez, Leivy P. Universidad de Guadalajara; MéxicoFil: Guerrero, Marisol. Hospital San José; ChileFil: Gutierrez-Rubio, Susan A. Universidad de Guadalajara; MéxicoFil: Jalfin, Beatriz. Hospital Regional de Agudos Eva Perón; ArgentinaFil: Lopez-Vazquez, Alejandra. Universidad de Sonora; MéxicoFil: Loria, Dora. Instituto de Oncología Angel Roffo; ArgentinaFil: Míguez, Silvia. Hospital Municipal de Oncología María Curie; ArgentinaFil: Moran-Mendoza, Andres de J. Hospital de Gineco-Obstetricia CMNO-IMSS; MéxicoFil: Morgan-Villela, Gilberto. Hospital de Especialidades. CMNO-IMSS; MéxicoFil: Mussetti, Carina. Registro Nacional de Cancer; UruguayFil: Nagai, Maria Aparecida. Instituto de Câncer de São Paulo; BrasilFil: Oceguera-Villanueva, Antonio. Instituto Jalisciense de Cancerologia; MéxicoFil: Reis, Rui M. Hospital de Câncer de Barretos; BrasilFil: Retamales, Javier. Grupo Oncológico Cooperativo Chileno de Investigación; ChileFil: Rodriguez, Robinson. Hospital Central de las Fuerzas Armadas; UruguayFil: Rosales, Cristina, Hospital Municipal de Oncología María Curie; ArgentinaFil: Salas-Gonzalez, Efrain. Hospital San José; ChileFil: Segovia, Laura. Hospital Barros Luco Trudeau; ChileFil: Sendoya, Juan M. CONICET. Fundación Instituto Leloir,; ArgentinaFil: Silva-Garcia, Aida A. OPD Hospital Civil de Guadalajara. Universidad de Guadalajara; MéxicoFil: Viña, Stella. Instituto de Oncología Angel Roffo; ArgentinaFil: Zagame, Livia. Instituto Jalisciense de Cancerologia; MéxicoFil: Jones, Beth. Yale University. Yale School of Public Health; Estados UnidosFil: Szklo, Moysés. Johns Hopkins University. Johns Hopkins Bloomberg School of Public Health; Estados Unido