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| Main Authors: | , , , |
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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2412.08002 |
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| _version_ | 1866916518020775936 |
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| author | Kerrison, Emily F. Sadler, Elaine M. Moss, Vanessa A. Mahony, Elizabeth K. |
| author_facet | Kerrison, Emily F. Sadler, Elaine M. Moss, Vanessa A. Mahony, Elizabeth K. |
| contents | We present here a study of the broadband spectral properties of 33 sources detected in HI absorption as part of the ASKAP-FLASH Pilot Surveys. We outline our approach to spectral classification and discuss the correlation seen between spectral shape and the detection of HI absorption. We further consider the implications of the observed correlation on the spatial distribution of the neutral gas, and on the jet-gas interactions. Our results are evaluated in the context of the forthcoming, full ASKAP-FLASH survey and other large, untargeted searches of the radio sky. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_08002 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Why so young? A curious connection between the broadband flux and neutral gas content of AGN Kerrison, Emily F. Sadler, Elaine M. Moss, Vanessa A. Mahony, Elizabeth K. Astrophysics of Galaxies We present here a study of the broadband spectral properties of 33 sources detected in HI absorption as part of the ASKAP-FLASH Pilot Surveys. We outline our approach to spectral classification and discuss the correlation seen between spectral shape and the detection of HI absorption. We further consider the implications of the observed correlation on the spatial distribution of the neutral gas, and on the jet-gas interactions. Our results are evaluated in the context of the forthcoming, full ASKAP-FLASH survey and other large, untargeted searches of the radio sky. |
| title | Why so young? A curious connection between the broadband flux and neutral gas content of AGN |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2412.08002 |