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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 1.

Photometric and spectral evolution of the novae that show a transition from Fe II to He/N classes. For each nova, the left panel displays its AAVSO V light curve, and the right panels display zoomed-in views of the V light curve (upper), of the κFeII (blue) and κHe/N (red) coefficients (middle), and the κ coefficient (bottom). The gray dashed lines indicate the epochs of the available spectra.

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