Image Details

Choose export citation format:

Weighing Hidden Companions of Compact Object Candidates via Rotational Broadening

  • Authors: Rui Wang, Zhi-Xiang Zhang, Wei-Min Gu, Hao-Bin Liu, Tuan Yi, Zhong-Rui Bai

Rui Wang et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 6.

Example of spectral disentangling for the target J0341. Top panel: the original observed spectrum (blue), the reconstructed spectrum from the disentangling procedure (red), and the individual spectra of the primary (green) and secondary (orange) components. The secondary spectrum is rescaled by a factor of 2. Stellar template (black dashed line) corresponds to 1.39 M (Teff = 7017 K, ﹩\mathrm{log}g﹩ = 4.0, ﹩v\sin i=80\,{\rm{km}}\,{{\rm{s}}}^{-1}﹩). Bottom panel: the residuals between the reconstructed and observed spectra, showing that the disentangling reproduces the observed spectrum within the noise level.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse