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Probing the tidal disruption event iPTF16axa with CLOUDY and disc-wind models
We present both a disc-wind model on the optical/UV emission continuum and CLOUDY modelling on the spectral lines of the tidal disruption event (TDE) iPTF16axa to understand the disc-wind emission and the properties of the atmosphere that impacts the line luminosity of the TDE. Assuming the optical/...
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Published in: | arXiv.org 2022-11 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
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Summary: | We present both a disc-wind model on the optical/UV emission continuum and CLOUDY modelling on the spectral lines of the tidal disruption event (TDE) iPTF16axa to understand the disc-wind emission and the properties of the atmosphere that impacts the line luminosity of the TDE. Assuming the optical/UV emission from the wind due to the disc super-Eddington phase, we use the steady structured disc-wind model with a spherical wind with constant velocity to fit the observations on multiple days. The extracted parameters are stellar-mass \(M_{\star} = 6.20 \pm 1.19 M_{\odot}\), disc radiative efficiency \(\log_{\rm 10}(\eta) = -1.22 \pm 1.327\), wind inner radius \(r_l = (2.013 \pm 0.551) \times 10^{14}~{\rm cm}\) and velocity \(v_w = 18999.4 \pm 1785.1 ~{\rm km~s^{-1}}\). The photosphere temperature for wind emission is \( \sim 2 \times 10^4~{\rm K}\) and the disc single blackbody temperature is \(\sim 0.995 \times 10^5~{\rm K}\). We also perform CLOUDY modelling to explain the observed He and H line luminosities that estimate a wind inner radius \(r_l = 7.07 \times 10^{14}~{\rm cm}\) and velocity \(v_w = 1.3 \times 10^4~{\rm km~s^{-1}}\). The independent analyses of iPTF16axa using CLOUDY and disc-wind models show comparable results that agree with observations. The CLOUDY modelling finds that both the super solar abundance of He and a smaller He II line optical depth is responsible for the enhancement of He II line luminosity over the H\(\alpha\) line luminosity. The super-solar abundance of He II agrees with a relatively large stellar mass and suggests that the disrupted star might have been a red giant. |
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ISSN: | 2331-8422 |
DOI: | 10.48550/arxiv.2211.14458 |