B. Baschek, J. Koêppen, Markus Scholz, R. Wehrsě, A. Heck, C. Jaschek, M. Jaschek
Abstract
On a obtenu des spectres UV de plusieurs etoiles λBoo et candidates λBoo. Il est possible de differencier les etoiles λBoo des etoiles A normales sur des spectres de faible resolution par leurs fortes caracteristiques d'absorption a λλ1600, 1657(CI), 1931(CI) et 3040 A
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On a obtenu des spectres UV de plusieurs etoiles λBoo et candidates λBoo. Il est possible de differencier les etoiles λBoo des etoiles A normales sur des spectres de faible resolution par leurs fortes caracteristiques d'absorption a λλ1600, 1657(CI), 1931(CI) et 3040 A
Key concepts: Physics, Astrophysics, Lambda, Stars, Stellar atmosphere, Ultraviolet astronomy, Astronomical spectroscopy, Spectral line