Elemental abundances in the Hg - Mn star γ Corvi

نویسنده

  • L. Houziaux
چکیده

Spectral data obtained at ESO, Observatoire de Haute-Provence and with the IUE covering the 120 910 nm spectral range allowed us to determine the abundances of 21 elements in the atmosphere of themoderately fast rotatingHg-Mn star γ Corvi.We find that helium, carbon, nitrogen, magnesium, aluminium, silicium, sulfur, chromium, iron and nickel are underabundant with respect to solar values. Beryllium, boron, calcium, phosphorus, titanium, manganese, copper, zinc, gallium and yttrium are overabundant by factors up to 2.5 dex. The oxygen abundance is found to be solar. This pattern is not unusual among Hg-Mn objects.

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تاریخ انتشار 1997