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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/2403.14832 |
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| _version_ | 1866913277939810304 |
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| author | Rodriguez-Ardila, Alberto Fonseca-Faria, Marcos Antonio Santos, Denimara Dias dos Panda, Swayamtrupta Marinello, Murilo |
| author_facet | Rodriguez-Ardila, Alberto Fonseca-Faria, Marcos Antonio Santos, Denimara Dias dos Panda, Swayamtrupta Marinello, Murilo |
| contents | We use near-infrared (NIR) spectroscopy covering simultaneously the $zJHK$ bands to look for outflowing gas from the nuclear environment of 1H0707-495 taking advantage that this region is dominated by low-ionization broad line region (BLR) lines, most of them isolated. We detect broad components in HI, FeII and OI, at rest to the systemic velocity, displaying full width at half maximum (FWHM) values of ~500 km s$^{-1}$, consistent with its classification as a narrow-line Seyfert~1 AGN. Moreover, most lines display a conspicuous blue-asymmetric profile, modeled using a blueshifted component, whose velocity shift reaches up to ~826 km s$^{-1}$. This last feature can be interpreted in terms of outflowing gas already observed in X-ray and UV lines in 1H0707-495 but not detected before in the low-ionization lines. We discuss the relevance of our findings within the framework of the wind scenario already proposed for this source and suggest that the wind extends well into the narrow line region due to the observation of a blueshifted component in the forbidden line of [SIII] $λ$9531. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_14832 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | First detection of outflowing gas in the outskirts of the broad line region in 1H-0707-495 Rodriguez-Ardila, Alberto Fonseca-Faria, Marcos Antonio Santos, Denimara Dias dos Panda, Swayamtrupta Marinello, Murilo Astrophysics of Galaxies We use near-infrared (NIR) spectroscopy covering simultaneously the $zJHK$ bands to look for outflowing gas from the nuclear environment of 1H0707-495 taking advantage that this region is dominated by low-ionization broad line region (BLR) lines, most of them isolated. We detect broad components in HI, FeII and OI, at rest to the systemic velocity, displaying full width at half maximum (FWHM) values of ~500 km s$^{-1}$, consistent with its classification as a narrow-line Seyfert~1 AGN. Moreover, most lines display a conspicuous blue-asymmetric profile, modeled using a blueshifted component, whose velocity shift reaches up to ~826 km s$^{-1}$. This last feature can be interpreted in terms of outflowing gas already observed in X-ray and UV lines in 1H0707-495 but not detected before in the low-ionization lines. We discuss the relevance of our findings within the framework of the wind scenario already proposed for this source and suggest that the wind extends well into the narrow line region due to the observation of a blueshifted component in the forbidden line of [SIII] $λ$9531. |
| title | First detection of outflowing gas in the outskirts of the broad line region in 1H-0707-495 |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2403.14832 |