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Speckle Interferometry at the US Naval Observatory. X.

机译:美国海军天文台的斑点干涉法。 X。

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The results of 3047 speckle interferometric observations of double stars, made with the 26 inch (66 cm) refractor of the US Naval Observatory, are presented. Each speckle interferometric observation of a system represents a combination of over a thousand short-exposure images. These observations are averaged into 1572 mean relative positions and range in separation from 020 to 6286, with a median separation of 419. This is the 10th in a series of papers presenting measures obtained with this system and covers the period 2003 January 13 through 2003 December 1. Included in these data are nine older measures whose positions were previously deemed possibly aberrant but are no longer classified this way following a confirming observation. Four of these systems have new orbital elements, which are presented here as well.
机译:呈现了使用美国海军天文台的26英寸(66厘米)折射镜制成的双星的3047个散斑干涉测量观测结果。系统的每个散斑干涉测量观察都代表一千多个短曝光图像的组合。这些观测值平均分为1572个平均相对位置和分离范围(从020到6286),中位分离值为419。这是一系列使用该系统获得的测量结果的论文中的第十,涵盖2003年1月13日至2003年12月1.这些数据中包括九项较旧的度量,其位置以前被认为可能是异常的,但在确认观察后不再以这种方式分类。这些系统中有四个具有新的轨道元素,这里也介绍了这些元素。

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