Nitrogen excess in slowly-rotating β Cephei stars: deep mixing or diffusion?
نویسندگان
چکیده
منابع مشابه
Diffusion and Pulsations in Slowly Rotating B Stars
Diffusion in cool B stars of the main sequence has been shown to strongly affect opacities and convection in cool B stars of the main sequence. We show here that diffusion in B stars maintains or enhances the excitation of pulsations in these stars. This result conflicts with observations as cool B stars that show evidence of diffusion, the HgMn stars, are stable to the current detection level....
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ژورنال
عنوان ژورنال: Communications in Asteroseismology
سال: 2007
ISSN: 1021-2043,1021-2043
DOI: 10.1553/cia150s199