FLARE STARS—A FAVORABLE OBJECT FOR STUDYING MECHANISMS OF NONTHERMAL ASTROPHYSICAL PHENOMENA
Authors: E. Oks, and R. E. Gershberg
2016 The Astrophysical Journal81916.
Provider: AAS Journals
Caption: Figure 1.
Dependence of the reduced half-widths Δλ1/2 (n)/λn = gn 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.