三角视差
- 网络trigonometric parallax
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用中心重迭法归算恒星三角视差的迭代算法
An iteration algorithm of the stellar trigonometric parallax reduction with the central overlap technique
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本文用中心重迭法迭代算法归算BD+2°348的三角视差,得出其相对视差等于0“.0879±0”。
The trigonometric parallax of BD + 2 ° 348 is reduced by iteration algorithm with the central overlap technique .
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恒星三角视差测定的现状和展望
The Current Situation of Determination of Trigonometric Stellar Parallaxes and Its Perspective
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按赤经、赤纬方向测定三角视差的系统差问题
On the systematic difference between trigonometric parallaxes determined in right ascension and declination
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反射望远镜的恒星三角视差测定
On Determination of Trigonometric Stellar Parallaxes with Reflectors
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用佘山40厘米折射望远镜测定的BD+2°348的三角视差
Determination of the parallax of bd + 2 ° 348 with the ZO-SE 40-cm refractor
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三角视差在天体物理研究中的应用
Astrophysical Applications of Stellar Trigonometric Parallaxes
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1.56米天体测量望远镜主要用以测定暗弱恒星的三角视差。今后也拟以此望远镜作为激光测月的接收望远镜。
We have designed an astrometric telescope , 1.66 meter in diameter , for determining the trigonometric parallaxes of faint stars .