机译:A search for line intensity enhancements in the far-UV spectra of active late-type stars arising from opacity
Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, NI, United Kingdom;
Department of Physics and Astronomy, California State University, 18111 Nordhoff Street, Northridge, CA 91330, United States;
Department of Physics, Imperial College, London SW7 2BZ, United Kingdom;
atomic processes; formation; late-type; line; opacity; radiative transfer; stars; ultraviolet;