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Infrared and visual lunar occultations measurements of stellar diameters and new binary stars detections at the Calar Alto 1.5m telescope

机译:红外和视觉月球掩星测量恒星直径   在Calar alto 1.5米望远镜上发现了新的双星探测器

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摘要

We present a program of routine lunar occultations, at optical and near-IRwavelengths, recently started at the 1.5m Spanish telescope at the Calar AltoObservatory. Both a CCD and an infrared array detector are used. The program isaimed mainly at the detection and investigation of binary systems, althoughresults in other areas of stellar research are also anticipated. Occultations are reported for a total of 40 stars. Among these, SAO 164567,SAO 78258 and AG+24 788 have been discovered to be binaries, with projectedseparations as small as 0.006". Furthermore, binarity is suspected in the caseof SAO 78119 and SAO 79251. Additionally, the angular diameter of the late-typegiant 30 Psc and of the infrared star V349 Gem have been accurately measured,this latter for the first time. We finally evaluate the instrumentation performance in terms of limitingmagnitude and angular resolution, and discuss applications to largertelescopes.
机译:我们提出了在光学波长和近红外波长下的常规月球掩星程序,该程序最近在Calar Alto天文台的1.5m西班牙望远镜上启动。 CCD和红外阵列检测器均被使用。该程序主要针对二进制系统的检测和研究,尽管也有望在其他恒星研究领域取得成果。据报道,掩星总共有40颗星。其中,已发现SAO 164567,SAO 78258和AG + 24 788是二进制文件,预计分离小至0.006“。此外,在SAO 78119和SAO 79251的情况下,怀疑是二值性的。首次精确测量了30Psc型红外恒星和V349红外星Gem,最后根据极限幅值和角分辨率评估了仪器的性能,并讨论了在大型望远镜中的应用。

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