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A line identification study of the IUE SWP high dispersion spectrum of the UV-bright star Barnard 29 of Messier 13

A line identification study of the coaddition of three SWP high dispersion IUE exposures of the UV-bright star Barnard 29 of M 13 is presented. One of these images took two IUE shifts. The previous study by de Boer K. S. and Savage B. D. (1983, Astrophys. J., 265) is extended and both stellar and interstellar lines of C I, C II, C IV, N I, N III, O I, Al III, Si II, Si IV and S II, and interstellar lines of N IV, N V, Al II and Fe II and stellar lines of C III, O III, O IV, Si II, Si III, P III and S III are found. These lines are the strongest expected lines in a hot Population II star. Apparent intensity minima corresponding to interstellar features are noted, especially those matching a high velocity cloud found by de Boer and Savage