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首页> 外文期刊>The Astrophysical journal >CCD MEASUREMENTS OF DOUBLE AND MULTIPLE STARS AT NAO ROZHEN AND ASV IN 2011. FIVE LINEAR SOLUTIONS*
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CCD MEASUREMENTS OF DOUBLE AND MULTIPLE STARS AT NAO ROZHEN AND ASV IN 2011. FIVE LINEAR SOLUTIONS*

机译:NAO ROZHEN和ASV在2011年的双星和多星CCD测量。五种线性解决方案*

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Using the 2?m telescope of the Bulgarian National Astronomical Observatory at Rozhen, observations of 222 double or multiple stars were carried out during three nights in 2011. This is the sixth series of measurements of CCD frames of double and multiple stars obtained at Rozhen. Also in 2011, using the 0.6?m telescope of the Serbian Astronomical Station on the mountain of Vidojevica, observations of 208 double or multiple stars were carried out during six nights. This is the first series of measurements of CCD frames of double and multiple stars obtained at this station. In this paper, we present the results for the position angle and angular separation for 337 pairs and residuals for 72 pairs with published orbital elements or linear solutions. These observations have angular separations in the range from 137 to 17281, with a median angular separation of 766. We also present the recalculated linear solutions for four pairs and one linear solution that has been calculated for the first time.
机译:使用位于罗镇(Rozhen)的保加利亚国家天文台的2?m望远镜,在2011年的三个晚上进行了222颗双星或多颗恒星的观测。这是在罗镇获得的第六颗测量双星和多星CCD镜架的系列。同样在2011年,使用维多耶维卡山(Vidojevica)上塞尔维亚天文站的0.6?m望远镜,在六个晚上进行了208颗双星或多颗恒星的观测。这是该站获得的双星和多星CCD帧的第一个测量系列。在本文中,我们用已发布的轨道元素或线性解给出了337对位置角和角度间隔以及72对残差的结果。这些观测值的角距在137至17281之间,中位角距为766。我们还介绍了重新计算的四对线对解和一个线形解,这是第一次计算。

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