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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 6.

Fraction of the available spectra of the novae that show evolution from the Fe II–dominated to the He/N-dominated phase as a function of t2, when available. Open circles correspond to novae that exhibit jitters in their light curves.

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