LIMB-DARKENING EFFECTS OF STELLAR ANGULAR DIAMETER MEASUREMENT
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摘要: 讨论了恒星临边昏暗在恒星角直径测量中的影响.研究表明,相对于二项式近似而言,UD模型和线性模型均对恒星角直径测量有所低估,在线性临边昏暗系数较小时,这种影响最大,UD和线性近似与二项式近似的差别最多分别达25.5%和12.6%;而在线性系数值趋近于1时,其相互差别随之可以忽略.而新旧线性临边近似之间对于恒星角直径测量的影响似乎并不很大.最后我们认为非线性临边昏暗效应的影响不可忽略.Abstract: In this paper the influence of the limb-darkening effects on stellar angular diameter measurement were studied. It shows that both UD and linear results underestimate the value of angular diameter; the difference is larger at stronger limb-darkening effects (c0 - 0), the largest difference among UD, linear result and quadric approach are 25.5%, 12.6% respectively. While their differences can be ignored when co tended to one. However, the difference between new and old linear approach seems small, it thinks that the quadric limb-darkening effects should be considered in the measurement of the stellar angular diameter.
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