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Broadening and Redward Asymmetry of Hα Line Profiles Observed by LAMOST during a Stellar Flare on an M-type Star

  • Authors: Yuchuan Wu, Hechao Chen, Hui Tian, Liyun Zhang, Jianrong Shi, Han He, Hongpeng Lu, Yu Xu, Haifeng Wang

Yuchuan Wu et al 2022 The Astrophysical Journal 928 .

  • Provider: AAS Journals

Caption: Figure 4.

Time evolution of the fitting parameters. The top rows show the total flux of the Voigt function (I 0), the HWHM of the Gaussian component (﹩\sigma \sqrt{{\rm{ln}}4}﹩), and the HWHM of the Lorentzian component (γ) in the Voigt–Gauss function, respectively. The bottom row only shows the height (a n ), the centroid (m), and the HWHM (﹩s\sqrt{{\rm{ln}}2}﹩) in the Gaussian function for the last four spectra, where profile asymmetries are observed. In each panel, the error bars represent uncertainties calculated from the fitting errors.

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