{"id":5972,"date":"2021-01-21T12:00:00","date_gmt":"2021-01-21T11:00:00","guid":{"rendered":"https:\/\/www.ieec.cat\/flujos-relativistas-en-los-sistemas-binarios-de-alta-masa\/"},"modified":"2023-01-17T15:05:05","modified_gmt":"2023-01-17T14:05:05","slug":"flujos-relativistas-en-los-sistemas-binarios-de-alta-masa","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/es\/flujos-relativistas-en-los-sistemas-binarios-de-alta-masa\/","title":{"rendered":"Flujos relativistas en los sistemas binarios de alta masa"},"content":{"rendered":"<p>[et_pb_section fb_built=\u00bb1&#8243; fullwidth=\u00bbon\u00bb _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb background_image=\u00bb\/wp-content\/uploads\/2022\/04\/slider-corpo2.jpg\u00bb height=\u00bb114px\u00bb global_colors_info=\u00bb{}\u00bb][\/et_pb_section][et_pb_section fb_built=\u00bb1&#8243; _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb custom_margin=\u00bb||0px||false|false\u00bb custom_padding=\u00bb||0px||false|false\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_row _builder_version=\u00bb4.14.8&#8243; 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_dynamic_attributes=\u00bbcontent\u00bb _module_preset=\u00bbdefault\u00bb custom_margin=\u00bb0px||0px||false|false\u00bb custom_padding=\u00bb0px||0px||false|false\u00bb hover_enabled=\u00bb0&#8243; global_colors_info=\u00bb{}\u00bb sticky_enabled=\u00bb0&#8243;]@ET-DC@eyJkeW5hbWljIjp0cnVlLCJjb250ZW50IjoiY3VzdG9tX21ldGFfbHVnYXJfZXZlbnRvIiwic2V0dGluZ3MiOnsiYmVmb3JlIjoiIiwiYWZ0ZXIiOiIiLCJlbmFibGVfaHRtbCI6Im9mZiJ9fQ==@[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=\u00bb1&#8243; _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb custom_margin=\u00bb0px||||false|false\u00bb custom_padding=\u00bb0px||||false|false\u00bb top_divider_color=\u00bbRGBA(255,255,255,0)\u00bb top_divider_height=\u00bb0px\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_row _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_column type=\u00bb4_4&#8243; _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_image src=\u00bbhttps:\/\/www.ieec.cat\/wp-content\/uploads\/2022\/12\/1610965388_eb32b5a18658234252073641bf2bd8ca_2021_01_edgar_molina.jpg\u00bb alt=\u00bbRelativistic outflows in high-mass binary systems\u00bb title_text=\u00bbRelativistic outflows in high-mass binary systems\u00bb _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb width=\u00bb600px\u00bb module_alignment=\u00bbcenter\u00bb global_colors_info=\u00bb{}\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb]El investigador Edgar Molina, del Instituto de Ciencias del Cosmos (ICCUB), hablar&aacute; sobre los flujos de salida relativistas en los sistemas binarios de alta masa.<\/p>\n<p>Los flujos relativistas se producen en un n&uacute;mero de sistemas binarios cercanos que consisten en un objeto compacto (ya sea un agujero negro o una estrella de neutrones) y una estrella compa&ntilde;era no degenerada. Estos flujos son sitios eficientes para la aceleraci&oacute;n de part&iacute;culas y, por lo tanto, pueden emitir radiaci&oacute;n no t&eacute;rmica en una amplia gama de longitudes de onda, desde radio hasta rayos gamma de muy alta energ&iacute;a. Cuando la compa&ntilde;era es una estrella de alta masa, el viento de esta &uacute;ltima tiene una influencia significativa en la propagaci&oacute;n y emisi&oacute;n de los flujos. Explicar&eacute; las diferentes formas en que esta influencia se manifiesta centr&aacute;ndome en dos tipos de sistemas binarios: 1) microcuasares, donde las salidas son chorros impulsados por la acreci&oacute;n de materia sobre el objeto compacto, y 2) sistemas binarios p&uacute;lsares no acrecientes, en los que los flujos relativistas se producen por la interacci&oacute;n de los vientos estelar y p&uacute;lsar.[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>El investigador Edgar Molina, del Instituto de Ciencias del Cosmos (ICCUB), hablar&aacute; sobre los flujos de salida relativistas en los sistemas binarios de alta masa. Los flujos relativistas se producen en un n&uacute;mero de sistemas binarios cercanos que consisten en un objeto compacto (ya sea un agujero negro o una estrella de neutrones) y una [&hellip;]<\/p>\n","protected":false},"author":0,"featured_media":5967,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":"2880","footnotes":""},"categories":[95,73],"tags":[],"class_list":["post-5972","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-charla","category-eventos"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.5 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Flujos relativistas en los sistemas binarios de alta masa - IEEC<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/www.ieec.cat\/es\/flujos-relativistas-en-los-sistemas-binarios-de-alta-masa\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Flujos relativistas en los sistemas binarios de alta masa - IEEC\" \/>\n<meta property=\"og:description\" content=\"El investigador Edgar Molina, del Instituto de Ciencias del Cosmos (ICCUB), hablar&aacute; sobre los flujos de salida relativistas en los sistemas binarios de alta masa. 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