X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries
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arXiv
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| Autores principales: | , |
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| Formato: | Preprint |
| Publicado: |
2024
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| _version_ | 1866915076030595072 |
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| author | Weng, Shan-Shan Ji, Long |
| author_facet | Weng, Shan-Shan Ji, Long |
| contents | Accreting X-ray pulsars, located in X-ray binaries, are neutron stars with magnetic fields as strong as $B\sim10^{12\text{--}13}$ G. This review offers a concise overview of the accretion and radiation processes of X-ray pulsars and summarizes their rich observational features, particularly focusing on complex and variable temporal phenomena, spectral properties, and evolution, the new window for X-ray polarimetry and multi-wavelength advances. We also briefly discuss other related systems, i.e., gamma-ray binaries and pulsating ultraluminous X-ray sources. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_17275 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries Weng, Shan-Shan Ji, Long High Energy Astrophysical Phenomena Accreting X-ray pulsars, located in X-ray binaries, are neutron stars with magnetic fields as strong as $B\sim10^{12\text{--}13}$ G. This review offers a concise overview of the accretion and radiation processes of X-ray pulsars and summarizes their rich observational features, particularly focusing on complex and variable temporal phenomena, spectral properties, and evolution, the new window for X-ray polarimetry and multi-wavelength advances. We also briefly discuss other related systems, i.e., gamma-ray binaries and pulsating ultraluminous X-ray sources. |
| title | X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2412.17275 |