作者: Suzan Edwards , Stephen E. Strom
DOI: 10.1007/3-540-12907-3_174
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摘要: The nature of the peculiar emission properties T Tauri stars is examined in light contributions from regions designated as photospheres, chromosphere coronae, and extended envelopes which are often characterized by mass loss. Although some manifestations activity can be linked to vigorous solar-stellar phenomena characteristic cool low mass, other characteristics behavior exhibited a wide range young stellar objects.