Figure 1 from FLARE STARS—A FAVORABLE OBJECT FOR STUDYING MECHANISMS OF NONTHERMAL ASTROPHYSICAL PHENOMENA

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FLARE STARS—A FAVORABLE OBJECT FOR STUDYING MECHANISMS OF NONTHERMAL ASTROPHYSICAL PHENOMENA

Authors: E. Oks, and R. E. Gershberg

2016 The Astrophysical Journal 819 16.

Provider: AAS Journals

Caption: Figure 1.

Dependence of the reduced half-widths Δλ_1/2 (n)/λ_n = g_n on the principal quantum number n of the upper level for Balmer lines observed in the solar flares of 08.18.59 and of 09.26.63.

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