【摘要】 考虑δr≠0和偏心率e二次以上的高次项,采用星风质量吸积的角动量守恒模型,并根据由此模型推出的星风吸积质量及轨道参量变化方程,重新计算了ζCap系统在星风吸积过程中吸积的物质质量和轨道参量的变化,从而进一步证实在分离双星系统,钡星通过星风吸积模型与其伴星发生了质量传输.更多还原

【Abstract】 By taking account of δr≠0,and considering the square and higher power terms of orbital eccentricity e,through the equation of conservation of orbital angular momentum,orbital parameters equations on the mass change are re-deduced.The equations of the orbital parameters are used to calculate the evolution of the orbital parameters and amount of accreted matter to the Ba stars.Our model are applied to the system ζCap.The effects of the tangential velocity of the escaping matter on the parameters are discussed更多还原