On the Potential of Bright, Young Pulsars to Power Ultrahigh Gamma-Ray Sources
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
| Authors: | , , , |
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| Format: | article |
| Status: | Published version |
| Publication Date: | 2022 |
| Country: | España |
| Institution: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repository: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/273227 |
| Online Access: | http://hdl.handle.net/10261/273227 |
| Access Level: | Open access |
| Keyword: | Gamma-ray sources Pulsars Rotation powered pulsars Pulsar wind nebulae High energy astrophysics ddc:520 |
| Summary: | This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. |
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