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Filament formation in wind-cloud interactions - I. Spherical clouds in uniform magnetic fields
ArticleAbstract: Filamentary structures are ubiquitous in the interstellar medium, yet their formation, internal struPalabras claves:galaxies: starburst, ISM: clouds, ISM: Magnetic fields, MHD- methods: numerical, Stars: winds, outflowsAutores:Bicknel G.V., Crocker R.M., Federrath C., Parkin E.R., Wladimir E. Banda-BarragánFuentes:scopusFilament formation in wind-cloud interactions- II. Clouds with turbulent density, velocity, and magnetic fields
ArticleAbstract: We present a set of numerical experiments designed to systematically investigate how turbulence andPalabras claves:galaxies: starburst, ISM: clouds, ISM: Magnetic fields, methods: numerical, MHD, TurbulenceAutores:Bicknell G.V., Crocker R.M., Federrath C., Wladimir E. Banda-BarragánFuentes:scopusSensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
ArticleAbstract: The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. SoPalabras claves:(Stars:) supernovae: general, cosmic rays, Galactic PeVatrons, Gamma rays: General, methods: data analysis, Methods: statisticalAutores:A. Baquero Larriva, Acero F., Acharyya A., Adam R., Aguasca-Cabot A., Agudo I., Aguirre-Santaella A., Alfaro J., Aloisio R., Amati L., Amato E., Ambrosi G., Anguner E.O., Aramo C., Arcaro C., Armstrong T., Asano K., Ascasíbar Y., Aschersleben J., Backes M., Baktash A., Balazs C., Balbo M., Ballet J., Barrio J.A., Bastieri D., Batista R.A., Baxter J.R., Benbow W., Bernardos-Martín M.I., Bernete J., Berti A., Bertucci B., Beshley V., Bhattacharjee P., Bhattacharyya S., Biland A., Bissaldi E., Biteau J., Blanch-Bigas O., Bordas P., Bottacini E., Bregeon J., Brose R., Bucciantini N., Bulgarelli A., Capasso M., Caraveo P.A., Cardillo M., Carosi R., Casanova S., Cascone E., Cassol F., Catalani F., Cerruti M., Chadwick P., Chaty S., Chen A., Chernyakova M., Chiavassa A., Chudoba J., Coimbra-Araujo C., Conforti V., Contreras J.L., Costa A., Costantini H., Crespo N.Á., Cristofari P., Crocker R.M., De Almeida U.B., De Angelis A., De Caprio V., de Gouveia Dal Pino E.M., de Ona Wilhelmi E., Delgado C., della Volpe D., Depaoli D., Di Girolamo T., Di Pierro F., Di Tria R., Diebold S., Djuvsland J.I., Dolcetta R.A.C., Donini A., Doro M., Dos Anjos R.D.C., Dwarkadas V.V., D’Amico G., D’Ammando F., Einecke S., Elsässer D., Emery G., Evoli C., Falceta-Goncalves D., Fedorova E., Fegan S., Martins V.B., Souza V.d., Tjus J.B., Venere L.D.Fuentes:scopus