Three-dimensional orbit and physical parameters of HD 6840  

Three-dimensional orbit and physical parameters of HD 6840

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作  者:Xiao-Li Wang Shu-Lin Ren Yan-Ning Fu 

机构地区:[1]Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China [2]University of Chinese Academy of Sciences,Beijing 100049,China

出  处:《Research in Astronomy and Astrophysics》2016年第2期113-118,共6页天文和天体物理学研究(英文版)

基  金:supported by the National Natural Science Foundation of China(Grant Nos.11073059,10833001,11178006,11273066 and 11203086)

摘  要:HD 6840 is a double-lined visual binary with an orbital period of N7.5 years. By fitting the speckle interferometric measurements made by the 6 m BTA telescope and 3.5 m WIYN telescope, Balega et al. gave a preliminary astrometric orbital solution of the system in 2006. Recently, Griffin derived a precise spectroscopic orbital solution from radial velocities observed with OPH and Cambridge Coravel. However, due to the low precision of the determined orbital inclination, the derived component masses are not satisfying. By adding the newly collected astrometric data in the Fourth Catalog of Interferometric Measurements of Binary Stars, we give a three-dimensional orbit solution with high precision and derive the preliminary physical parameters of HD 6840 via a simultaneous fit including both astrometric and radial velocity measurements.HD 6840 is a double-lined visual binary with an orbital period of N7.5 years. By fitting the speckle interferometric measurements made by the 6 m BTA telescope and 3.5 m WIYN telescope, Balega et al. gave a preliminary astrometric orbital solution of the system in 2006. Recently, Griffin derived a precise spectroscopic orbital solution from radial velocities observed with OPH and Cambridge Coravel. However, due to the low precision of the determined orbital inclination, the derived component masses are not satisfying. By adding the newly collected astrometric data in the Fourth Catalog of Interferometric Measurements of Binary Stars, we give a three-dimensional orbit solution with high precision and derive the preliminary physical parameters of HD 6840 via a simultaneous fit including both astrometric and radial velocity measurements.

关 键 词:BINARIES spectroscopic -- astrometry -- stars fundamental parameters -- stars individual (HD 6840) 

分 类 号:P135[天文地球—天体力学]

 

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