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Continuum and Line Emission of Flares on Red Dwarf Stars: Origin of the Blue Continuum Radiationстатья
- Автор: Morchenko E.S.
- Сборник: Radiation mechanisms of astrophysical objects: classics today
- Серия: Proceedings of the conference in honor of the 100th birthday of Academician V.V. Sobolev held at St. Petersburg on September 21-25, 2015
- Год издания: 2017
- Место издания: Edit Print publishing house Yerevan
- Первая страница: 219
- Последняя страница: 221
- Аннотация: There are two types of models that explain the appearance of the quasi- blackbody radiation during the impulsive phase of stellar flares. Grinin and Sobolev (Astrophysics, Vol. 13, 348, 1977) argue that this component of the optical continuum is formed in “the transition layer between the chromosphere and the photosphere.” Katsova et al. (Astrophysics, Vol. 17, 156, 1981) have “raised” the source of the white-light continuum up to the dense region in the perturbed chromosphere. In the present contribution (the main paper is published in “Astrophysics”), we show that the statement in (Astrophysics, Vol. 17, 156, 1981) is erroneous.
- Добавил в систему: Морченко Егор Сергеевич
Прикрепленные файлы
| № | Имя | Описание | Имя файла | Размер | Добавлен |
|---|---|---|---|---|---|
| 1. | Полный текст | p219_Morchenko.pdf | 171,6 КБ | 26 октября 2022 [Morchenko] | |
| 2. | Morchenko-2015.png | Morchenko-2015.png | 134,4 КБ | 21 ноября 2022 [Morchenko] |