Abstract
Among the strongest lines from stellar transition regions are the resonance lines of N V (1240Å), Si IV (1394, 1403Å), and C IV (1549Å), which are all observable by the IUE.
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References
Jordan, C., 1969, MNRAS, 142 501
Saxner, M., 1981, Astron. Astrophys., 104, 240
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© 1983 Springer Science+Business Media Dordrecht
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Saxner, M. (1983). Some Properties of Stellar Transition Regions. In: Byrne, P.B., Rodonò, M. (eds) Activity in Red-Dwarf Stars. Astrophysics and Space Science Library, vol 102. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7157-8_11
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DOI: https://doi.org/10.1007/978-94-009-7157-8_11
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