JAT, MAG, and GR-L are supported by the Direccion General de Asuntos del Personal Academico (DGAPA, UNAM) through the Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPIIT) projects IA100318 and IA100720. MAG acknowledges support from grant PGC2018102184-B-I00, cofunded with FEDER funds. GR-L acknowledges support from Consejo Nacional de Ciencia y Tecnologia (CONACYT) and Programa para el Desarrollo Profesional (PRODEP), Mexico. LS acknowledges support from DGAPA, UNAM PAPIIT project IN101819. Thiswork hasmade extensive use of theNASA's Astrophysics Data System. ES thanks CONACYT (Mexico) for a research studentship. Thisworkwas based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. The scientific results reported in this paper are based on observations made by the Chandra X-ray Observatory and published previously in cited articles.

中文翻译：

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来自经典新星 DQ Her 的扩展 X 射线发射——关于磁化射流的可能存在

JAT、MAG 和 GR-L 由 Direccion General de Asuntos del Personal Academico (DGAPA, UNAM) 通过 Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPIIT) 项目 IA100318 和 IA100720 提供支持。MAG 承认与 FEDER 基金共同资助的赠款 PGC2018102184-B-I00 的支持。GR-L 感谢墨西哥国家科学和技术委员会 (CONACYT) 和 Programa para el Desarrollo Profesional (PRODEP) 的支持。LS 感谢 DGAPA、UNAM PAPIIT 项目 IN101819 的支持。这项工作广泛使用了美国宇航局的天体物理学数据系统。ES 感谢 CONACYT（墨西哥）提供研究奖学金。这项工作基于通过 XMM-Newton 获得的观测结果，这是一项 ESA 科学任务，其仪器和捐款由 ESA 成员国和 NASA 直接资助。