A Multi-Mechanism Hybrid Model of Peaked-Spectrum Radio Sources
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arXiv
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| Autores principales: | , , , , , , , , |
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| Formato: | Preprint |
| Publicado: |
2025
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| Materias: | |
| Acceso en línea: | |
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| _version_ | 1866913854310580224 |
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| author | Sun, Guang-Chen Li, Yichao Deng, Furen Cong, Yanping An, Fangxia Zhang, Jiajun Wang, Yougang Zhang, Xin Chen, Xuelei |
| author_facet | Sun, Guang-Chen Li, Yichao Deng, Furen Cong, Yanping An, Fangxia Zhang, Jiajun Wang, Yougang Zhang, Xin Chen, Xuelei |
| contents | The peaked-spectrum (PS) sources exhibit turnover characteristics in their broad radio spectra. However, the mechanism underlying this phenomenon remains elusive. The two most common hypotheses are synchrotron self-absorption (SSA) and free-free absorption (FFA). By incorporating multiple absorption scenarios, we propose a multi-mechanism hybrid (MMH) model, which aligns well with current observational data and provides a good physical explanation. Using the GLEAM survey data, we identified a sample of 4,315 sources with peak frequencies approximately between 72--3000 MHz, most of which are MHz-peaked-spectrum sources (MPS). Our analysis shows that instead of SSA, the FFA is the dominant mechanism in producing the spectral turnover for most of the sources in this sample. The index of the optically thick spectrum alpha_thick has a lower boundary due to the FFA, and the steeper alpha_thick indicates a complex multi-absorption mechanism. In particular, the external FFA produces substantial alpha_thick, which exhibits a weak correlation with the peak frequency. Future ultra-long wavelength observations would also provide data on the spectrum of these sources at even lower frequencies. Determining the absorption mechanism that shaped the spectrum of these sources would be a crucial part of understanding their nature. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2504_04387 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | A Multi-Mechanism Hybrid Model of Peaked-Spectrum Radio Sources Sun, Guang-Chen Li, Yichao Deng, Furen Cong, Yanping An, Fangxia Zhang, Jiajun Wang, Yougang Zhang, Xin Chen, Xuelei Astrophysics of Galaxies The peaked-spectrum (PS) sources exhibit turnover characteristics in their broad radio spectra. However, the mechanism underlying this phenomenon remains elusive. The two most common hypotheses are synchrotron self-absorption (SSA) and free-free absorption (FFA). By incorporating multiple absorption scenarios, we propose a multi-mechanism hybrid (MMH) model, which aligns well with current observational data and provides a good physical explanation. Using the GLEAM survey data, we identified a sample of 4,315 sources with peak frequencies approximately between 72--3000 MHz, most of which are MHz-peaked-spectrum sources (MPS). Our analysis shows that instead of SSA, the FFA is the dominant mechanism in producing the spectral turnover for most of the sources in this sample. The index of the optically thick spectrum alpha_thick has a lower boundary due to the FFA, and the steeper alpha_thick indicates a complex multi-absorption mechanism. In particular, the external FFA produces substantial alpha_thick, which exhibits a weak correlation with the peak frequency. Future ultra-long wavelength observations would also provide data on the spectrum of these sources at even lower frequencies. Determining the absorption mechanism that shaped the spectrum of these sources would be a crucial part of understanding their nature. |
| title | A Multi-Mechanism Hybrid Model of Peaked-Spectrum Radio Sources |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2504.04387 |