Rates of Energy Gain and Loss in the Circumstellar Envelopes of Be Stars


We have investigated the rates of energy gain and energy loss in the envelopes of Be stars in order to determine the temperature distribution self-consistently. Using our models, we have successfully matched the relative line strengths of H for both an early Be star, Cas, and a late Be star, 1 Delphini, with the envelope temperature determined via energy… (More)


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