Modelling the thermal and non-thermal emissions of the supernova remnant 3C 397
The data underlying this article will be shared on reasonable request to the corresponding author. This work uses material obtained from: the NASA/SAO Chandra Data Archive (CDA), the MIPSGAL survey obtained with the Spitzer Space Telescope, which was operated by the Jet Propulsion Laboratory, Califo...
| Autores: | , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/403143 |
| Acceso en línea: | http://hdl.handle.net/10261/403143 https://api.elsevier.com/content/abstract/scopus_id/105013756159 |
| Access Level: | acceso abierto |
| Palabra clave: | ISM: supernova remnants Methods: numerical MHD Shock waves |
| Sumario: | The data underlying this article will be shared on reasonable request to the corresponding author. This work uses material obtained from: the NASA/SAO Chandra Data Archive (CDA), the MIPSGAL survey obtained with the Spitzer Space Telescope, which was operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA, and MeerKat survey. The South African Radio Astronomy Observatory, a facility of the National Research Foundation, an agency of the Department of Science and Innovation, operates the MeerKAT telescope. |
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