Figure 6 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 6.

Dependence of the reduced half-widths Δλ_1/2 (n)/λ_n on the principal quantum number n of the upper level for Balmer lines observed by Gershberg & Shakhovskaja (1971) in the flare of AD Leo of 03.02.70 in spectrum #1 (dots). The average trend is shown by the dashed line.

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