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| Main Authors: | , , , , , , , |
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| Format: | Preprint |
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2023
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| Online Access: | https://arxiv.org/abs/2306.13930 |
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| _version_ | 1866909091818897408 |
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| author | Nagoshi, Shumpei Iwamuro, Fumihide Yamada, Satoshi Ueda, Yoshihiro Oikawa, Yuto Otsuka, Masaaki Isogai, Keisuke Mineshige, Shin |
| author_facet | Nagoshi, Shumpei Iwamuro, Fumihide Yamada, Satoshi Ueda, Yoshihiro Oikawa, Yuto Otsuka, Masaaki Isogai, Keisuke Mineshige, Shin |
| contents | The physical origins of quasar components, such as the broad line region (BLR) and dust torus, remain under debate. To gain insights into them, we focused on Changing-State Quasars (CSQs) which provide a unique perspective through structural changes associated with accretion disk state transitions. We targeted SDSS J125809.31+351943.0, an extremely variable CSQ, to study its central core structure and kinematics. We conducted reverberation mapping with optical spectroscopy to explore the structure of the BLR and estimate the black hole mass. The results from H$β$ reverberation mapping indicated a black hole mass of $10^{9.64^{+0.11}_{-0.20}}\rm{M_\odot}$. Additionally, we analyzed variations in the optical to X-ray spectral indices, $α_{\rm{ox}}$, before and after the state transition, to investigate the accretion disk. These variations in $α_{\rm{ox}}$ and the Eddington ratio (from 0.4 \% to 2.4 \%) exhibitied behavior similar to state transitions observed in X-ray binary systems. Spectral analysis of H$β$ revealed a predominantly double-peaked profile during dim periods, transitioning to include a single-peaked component as the quasar brightened, suggesting that H$β$ contains a mixture of two components. Each of these components has its distinct characteristics: the first is a double-peaked profile that remains stable despite changes in the accretion rate, while the second is a variable single-peaked profile. Using time lags from reverberation mapping, we estimated the spatial relationships between these BLR components, the accretion disk, and the dust torus. Our results suggest that the BLR consists of two distinct components, each differing in location and origin. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2306_13930 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Probing the origin of the two-component structure of broad line region by reverberation mapping of an extremely variable quasar Nagoshi, Shumpei Iwamuro, Fumihide Yamada, Satoshi Ueda, Yoshihiro Oikawa, Yuto Otsuka, Masaaki Isogai, Keisuke Mineshige, Shin Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena The physical origins of quasar components, such as the broad line region (BLR) and dust torus, remain under debate. To gain insights into them, we focused on Changing-State Quasars (CSQs) which provide a unique perspective through structural changes associated with accretion disk state transitions. We targeted SDSS J125809.31+351943.0, an extremely variable CSQ, to study its central core structure and kinematics. We conducted reverberation mapping with optical spectroscopy to explore the structure of the BLR and estimate the black hole mass. The results from H$β$ reverberation mapping indicated a black hole mass of $10^{9.64^{+0.11}_{-0.20}}\rm{M_\odot}$. Additionally, we analyzed variations in the optical to X-ray spectral indices, $α_{\rm{ox}}$, before and after the state transition, to investigate the accretion disk. These variations in $α_{\rm{ox}}$ and the Eddington ratio (from 0.4 \% to 2.4 \%) exhibitied behavior similar to state transitions observed in X-ray binary systems. Spectral analysis of H$β$ revealed a predominantly double-peaked profile during dim periods, transitioning to include a single-peaked component as the quasar brightened, suggesting that H$β$ contains a mixture of two components. Each of these components has its distinct characteristics: the first is a double-peaked profile that remains stable despite changes in the accretion rate, while the second is a variable single-peaked profile. Using time lags from reverberation mapping, we estimated the spatial relationships between these BLR components, the accretion disk, and the dust torus. Our results suggest that the BLR consists of two distinct components, each differing in location and origin. |
| title | Probing the origin of the two-component structure of broad line region by reverberation mapping of an extremely variable quasar |
| topic | Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2306.13930 |