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A Quantitative Method to Investigate the Spectral Class Time Evolution of Novae

  • Authors: M. Kopsacheili, M. Guerrero, D.A. Vasquez-Torres

M. Kopsacheili et al 2026 The Astrophysical Journal 1012 .

  • Provider: AAS Journals

Caption: Figure 5.

Upper panel: V light curves of the recurrent novae of our sample. Lower panel: evolution of κFeII (blue) and κHe/N (red). The gray dashed lines indicate the epochs of the available spectra. Note that for RS Oph, the Fe II flux in the first spectrum is null. Consequently, the corresponding blue point is not shown because the y-axis is on a logarithmic scale.

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