In this study,the apsidal motion analyses of the eclipsing binary systems V398 Lac,V2544 Cyg,and V785 Cas are presented.The(O-C)diagrams of the selected systems were constructed using all available and reliable times ...In this study,the apsidal motion analyses of the eclipsing binary systems V398 Lac,V2544 Cyg,and V785 Cas are presented.The(O-C)diagrams of the selected systems were constructed using all available and reliable times of minimum light compiled from the literature.As a result,the apsidal motion periods were determined to be 353±50 yr,43.3±5.1 yr and 83.4±8.5 yr,respectively.Furthermore,the TESS light curves of the three systems were analyzed to derive their photometric and absolute parameters.The component masses were determined as follows:for V398 Lac,M_(1)=3.83±0.35 M_(⊙)and M2=3.27±0.35 M_(⊙);for V2544 Cyg,M_(1)=1.75±0.38 M_(⊙)and M2=1.40±0.38 M_(⊙);for V785 Cas,M_(1)=5.64±0.41 M_(⊙)and M2=5.18±0.41 M_(⊙).The parameters related to apsidal motion,as well as the observational and theoretical internal structure constants(K_(2,obs) and K_(2,teo))were calculated for studied binaries.The relativistic contribution to the observed apsidal motion rate was found to be relatively small,constituting less than approximately 5%of the total rate in each system.The theoretical internal structure constants were derived from the evolutionary models,assuming a standard chemical composition of(X,Z)=(0.70,0.01).展开更多
针对网络化控制系统(NCS)中的随机时变时延,采用自行开发的基于应用层的测试软件,按照IETF(The Internet Engi-neering Task Force)的RFC2544规范,进行了6个多月实际测量,获得了170余万个网络时延数据;通过对实验数据进行相关分析,建立...针对网络化控制系统(NCS)中的随机时变时延,采用自行开发的基于应用层的测试软件,按照IETF(The Internet Engi-neering Task Force)的RFC2544规范,进行了6个多月实际测量,获得了170余万个网络时延数据;通过对实验数据进行相关分析,建立了网络时延的自适应自回归(AR)模型;并用自适应最小均方差(LMS)算法对实测的网络时延进行了估计和预测,实验结果表明了算法的有效性。展开更多
基金Funding for TESS is provided by the NASA Science Mission Directorate。
文摘In this study,the apsidal motion analyses of the eclipsing binary systems V398 Lac,V2544 Cyg,and V785 Cas are presented.The(O-C)diagrams of the selected systems were constructed using all available and reliable times of minimum light compiled from the literature.As a result,the apsidal motion periods were determined to be 353±50 yr,43.3±5.1 yr and 83.4±8.5 yr,respectively.Furthermore,the TESS light curves of the three systems were analyzed to derive their photometric and absolute parameters.The component masses were determined as follows:for V398 Lac,M_(1)=3.83±0.35 M_(⊙)and M2=3.27±0.35 M_(⊙);for V2544 Cyg,M_(1)=1.75±0.38 M_(⊙)and M2=1.40±0.38 M_(⊙);for V785 Cas,M_(1)=5.64±0.41 M_(⊙)and M2=5.18±0.41 M_(⊙).The parameters related to apsidal motion,as well as the observational and theoretical internal structure constants(K_(2,obs) and K_(2,teo))were calculated for studied binaries.The relativistic contribution to the observed apsidal motion rate was found to be relatively small,constituting less than approximately 5%of the total rate in each system.The theoretical internal structure constants were derived from the evolutionary models,assuming a standard chemical composition of(X,Z)=(0.70,0.01).
基金国家自然科学基金(the National Natural Science Foundation of China under Grant No.60674057)
文摘针对网络化控制系统(NCS)中的随机时变时延,采用自行开发的基于应用层的测试软件,按照IETF(The Internet Engi-neering Task Force)的RFC2544规范,进行了6个多月实际测量,获得了170余万个网络时延数据;通过对实验数据进行相关分析,建立了网络时延的自适应自回归(AR)模型;并用自适应最小均方差(LMS)算法对实测的网络时延进行了估计和预测,实验结果表明了算法的有效性。
