Simultaneous Optical to X-ray Spectra of OJ 287: Insights into X-ray spectral changes and particle spectra
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arXiv
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| Formato: | Preprint |
| Publicado: |
2024
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| _version_ | 1866908526068105216 |
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| author | Kushwaha, Pankaj |
| author_facet | Kushwaha, Pankaj |
| contents | OJ 287 is one of the most dynamic BL Lacertae objects that has exhibited behaviour representative of the entire blazar class and is also one of the best sources with simultaneous multi-wavelength coordinated data. Motivated by strong X-ray variability exhibited by the source, we systematically investigated the simultaneous optical to X-ray emission of the source with a focus on the spectral state of the lowest recorded X-ray flux state to understand the X-ray spectral changes. The optical-UV emission being synchrotron, the associated spectral variation is a direct reflection of the high-energy end of the underlying particle spectrum and its power-law continuation to X-rays can drastically affect the X-ray spectrum without much change in optical flux. Thus the combined optical to X-ray provides a potential tool to investigate and explore particle spectrum as well as highest particle energies. We report the finding of a power-law optical-UV spectrum with a photon spectral index of 2.71 $\pm$ 0.03 continuing to X-ray energies and accounting for this contribution at X-ray results in a photon spectral index of 1.15-1.3. We discuss the possible implications of this on X-ray spectral variations and the particle spectrum. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_05783 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Simultaneous Optical to X-ray Spectra of OJ 287: Insights into X-ray spectral changes and particle spectra Kushwaha, Pankaj High Energy Astrophysical Phenomena Astrophysics of Galaxies OJ 287 is one of the most dynamic BL Lacertae objects that has exhibited behaviour representative of the entire blazar class and is also one of the best sources with simultaneous multi-wavelength coordinated data. Motivated by strong X-ray variability exhibited by the source, we systematically investigated the simultaneous optical to X-ray emission of the source with a focus on the spectral state of the lowest recorded X-ray flux state to understand the X-ray spectral changes. The optical-UV emission being synchrotron, the associated spectral variation is a direct reflection of the high-energy end of the underlying particle spectrum and its power-law continuation to X-rays can drastically affect the X-ray spectrum without much change in optical flux. Thus the combined optical to X-ray provides a potential tool to investigate and explore particle spectrum as well as highest particle energies. We report the finding of a power-law optical-UV spectrum with a photon spectral index of 2.71 $\pm$ 0.03 continuing to X-ray energies and accounting for this contribution at X-ray results in a photon spectral index of 1.15-1.3. We discuss the possible implications of this on X-ray spectral variations and the particle spectrum. |
| title | Simultaneous Optical to X-ray Spectra of OJ 287: Insights into X-ray spectral changes and particle spectra |
| topic | High Energy Astrophysical Phenomena Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2410.05783 |