Outflow-cloud interaction as the possible origin of the peculiar radio emission in the tidal disruption event AT2018cqh
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arXiv
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| Auteurs principaux: | , , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866914057958719488 |
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| author | Yang, Lei Shu, Xinwen Mou, Guobin Xue, Yongquan Sun, Luming Zhang, Fabao Zhang, Zhumao Wang, Yibo Wu, Tao Jiang, Ning Ding, Hucheng Wang, Tinggui |
| author_facet | Yang, Lei Shu, Xinwen Mou, Guobin Xue, Yongquan Sun, Luming Zhang, Fabao Zhang, Zhumao Wang, Yibo Wu, Tao Jiang, Ning Ding, Hucheng Wang, Tinggui |
| contents | AT2018cqh is a unique optical tidal disruption event (TDE) discovered in a dwarf galaxy exhibiting delayed X-ray and radio flares. We present the results from high-resolution VLBA and e-MERLIN radio observations of AT2018cqh extending to $δ$t $\sim$ 2250 days post discovery, which reveal a compact radio emission, unresolved at a scale of <~ 0.13 pc at 7.6 GHz, with a high brightness temperature of $T_b$ ~> 4.03 $\times$ 10$^{9}$ K. The radio spectral energy distribution (SED) is found to gradually shift towards a higher peak flux density and frequency over a period of $\sim$1000 days. An equipartition analysis suggests that there is a little change in the radio emitting region over this period, while the electron density increases by a factor of 3. The radio light curve at 0.89 GHz continues to rise, with a bump feature lasting for 240 days. These properties are in contrast to the predictions of standard shockwave model from a diffuse circumnuclear medium, but could be explained if dense clouds exist in the circumnuclear environment. The latter scenario is supported by our hydrodynamic simulations of the interaction of TDE outflow with a cloud, which can reproduce the temporal evolution in the radio SED. This work highlights the importance of the outflow-cloud interaction in explaining the delayed, fast-rising radio emission observed in some TDEs, especially those occurring in galaxies with pre-existing AGN activity. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_21299 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Outflow-cloud interaction as the possible origin of the peculiar radio emission in the tidal disruption event AT2018cqh Yang, Lei Shu, Xinwen Mou, Guobin Xue, Yongquan Sun, Luming Zhang, Fabao Zhang, Zhumao Wang, Yibo Wu, Tao Jiang, Ning Ding, Hucheng Wang, Tinggui High Energy Astrophysical Phenomena Astrophysics of Galaxies AT2018cqh is a unique optical tidal disruption event (TDE) discovered in a dwarf galaxy exhibiting delayed X-ray and radio flares. We present the results from high-resolution VLBA and e-MERLIN radio observations of AT2018cqh extending to $δ$t $\sim$ 2250 days post discovery, which reveal a compact radio emission, unresolved at a scale of <~ 0.13 pc at 7.6 GHz, with a high brightness temperature of $T_b$ ~> 4.03 $\times$ 10$^{9}$ K. The radio spectral energy distribution (SED) is found to gradually shift towards a higher peak flux density and frequency over a period of $\sim$1000 days. An equipartition analysis suggests that there is a little change in the radio emitting region over this period, while the electron density increases by a factor of 3. The radio light curve at 0.89 GHz continues to rise, with a bump feature lasting for 240 days. These properties are in contrast to the predictions of standard shockwave model from a diffuse circumnuclear medium, but could be explained if dense clouds exist in the circumnuclear environment. The latter scenario is supported by our hydrodynamic simulations of the interaction of TDE outflow with a cloud, which can reproduce the temporal evolution in the radio SED. This work highlights the importance of the outflow-cloud interaction in explaining the delayed, fast-rising radio emission observed in some TDEs, especially those occurring in galaxies with pre-existing AGN activity. |
| title | Outflow-cloud interaction as the possible origin of the peculiar radio emission in the tidal disruption event AT2018cqh |
| topic | High Energy Astrophysical Phenomena Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2509.21299 |