摘要
利用光变模型对收集到的30个Blazars的光曲线进行拟合,由模型参数确定光变特征时标。根据确定的光变特征时标计算了中心天体质量和辐射区域上限,结果表明利用光变模型得到的特征时标与其他研究者的结果相符。因此,该光变模型可以作为研究Blazar短时标光变的一种新的方法。
By using light model,the paper fit the light curve to the 30 Blazars of collection,and acquire the characteristic timescale by model parameter.It is possible to estimate a black hole of emitting region R from the timescale.Comparing the result of others,we can obtain that these characteristic timescale acquired by the light model correspond to the result of others.So this light model can be a new method for researching the short timescale of blazer.
出处
《云南师范大学学报（自然科学版）》
2011年第3期12-19,共8页
Journal of Yunnan Normal University:Natural Sciences Edition
