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The spectrum of the Bp star HD 36916

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Abstract

The spectrum of the peculiar Bp star HD 36916 has been studied on plates with dispersion 9.7 A/mm and compared with those of η Aur, B3V andi And, B8V. A comparison of the observed contours of Hβ, Hγ and of the Balmer discontinuity D with those computed by Mihalas gives the following results: HD 36916: θe=0.347, logg=3.8;i And: θe=0.383, logg=3.2; η Aur: θe=0.302, logg=3.6. HD 36916 presents the characteristics of the Si-λ4200 stars: strong deficiency in helium and probably also in oxygen and nitrogen, strong excess of silicon and strontium; 3984 Hgii is present. Moreover this star also has characteristics which are not common to Si-λ4200 stars but rather to Mn stars: excess by a factor of ten of the elements of the iron group and an excess larger, probably of the order of 100, for manganese. The star is a member of the Sword subgroup of the Orion association.

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Hack, M. The spectrum of the Bp star HD 36916. Astrophys Space Sci 5, 403–419 (1969). https://doi.org/10.1007/BF00652389

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  • DOI: https://doi.org/10.1007/BF00652389

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