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pro vyhledávání: '"Donne, Dion"'
Autor:
Donné, Dion, Keppens, Rony
The mass cycle of solar prominences or filaments is still not completely understood. Researchers agree that these dense structures form by coronal in-situ condensations and plasma siphoning from the underlying chromosphere. In the evaporation-condens
Externí odkaz:
http://arxiv.org/abs/2405.20048
Autor:
Maes, Silke, Siess, Lionel, Homan, Ward, Malfait, Jolien, De Ceuster, Frederik, Ceulemans, Thomas, Donne, Dion, Esseldeurs, Mats, Decin, Leen
Low- and intermediate mass stars experience a significant mass loss during the last phases of their evolution, which obscures them in a vast, dusty envelope. Although it has long been thought this envelope is generally spherically symmetric in shape,
Externí odkaz:
http://arxiv.org/abs/2206.12278