Application of the Disk Instability Model to All Quasiperiodic Eruptions
After the first quasiperiodic eruption (QPE; GSN 069) was reported in 2019, four other sources have been identified as a QPE or a candidate. However, the physics behind QPEs is still unclear, although several models have been proposed. Pan et al. proposed an instability model for an accretion disk w...
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| Vydané v: | The Astrophysical journal Ročník 952; číslo 1; s. 32 - 37 |
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| Hlavní autori: | , , |
| Médium: | Journal Article |
| Jazyk: | English |
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Philadelphia
The American Astronomical Society
01.07.2023
IOP Publishing |
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| ISSN: | 0004-637X, 1538-4357 |
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| Abstract | After the first quasiperiodic eruption (QPE; GSN 069) was reported in 2019, four other sources have been identified as a QPE or a candidate. However, the physics behind QPEs is still unclear, although several models have been proposed. Pan et al. proposed an instability model for an accretion disk with magnetically driven outflows in the first QPE of GSN 069, which is able to reproduce both the light curve and the evolution of the spectra fairly well. In this work, we extend this model to all QPEs. We improve the calculations of the spectrum of the disk by introducing a hardening factor, which is caused by a deviation of opacity from a blackbody. We find that the light curves and evolution of the spectra of the four QPEs and candidates can all be well reproduced by our model calculations. |
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| AbstractList | After the first quasiperiodic eruption (QPE; GSN 069) was reported in 2019, four other sources have been identified as a QPE or a candidate. However, the physics behind QPEs is still unclear, although several models have been proposed. Pan et al. proposed an instability model for an accretion disk with magnetically driven outflows in the first QPE of GSN 069, which is able to reproduce both the light curve and the evolution of the spectra fairly well. In this work, we extend this model to all QPEs. We improve the calculations of the spectrum of the disk by introducing a hardening factor, which is caused by a deviation of opacity from a blackbody. We find that the light curves and evolution of the spectra of the four QPEs and candidates can all be well reproduced by our model calculations. |
| Author | Cao, Xinwu Li, Shuang-Liang Pan, Xin |
| Author_xml | – sequence: 1 givenname: Xin orcidid: 0000-0002-6938-3594 surname: Pan fullname: Pan, Xin organization: University of Chinese Academy of Sciences , 19A Yuquan Road, Beijing 100049, People’s Republic of China – sequence: 2 givenname: Shuang-Liang orcidid: 0000-0002-7299-4513 surname: Li fullname: Li, Shuang-Liang organization: Shanghai Astronomical Observatory Key Laboratory for Research in Galaxies and Cosmology, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, , People’s Republic of China – sequence: 3 givenname: Xinwu orcidid: 0000-0002-2355-3498 surname: Cao fullname: Cao, Xinwu organization: Zhejiang University Institute for Astronomy, Zhejiang Institute of Modern Physics, School of Physics, 866 Yuhangtang Rd, Hangzhou 310058, People’s Republic of China |
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| Snippet | After the first quasiperiodic eruption (QPE; GSN 069) was reported in 2019, four other sources have been identified as a QPE or a candidate. However, the... |
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| SubjectTerms | Accretion disks Active galactic nuclei Astrophysics Blackbody Evolution Galaxy accretion disks Light curve Magnetic fields Modelling Opacity Spectra |
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| Title | Application of the Disk Instability Model to All Quasiperiodic Eruptions |
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