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Suspected Variables in AAVSO Star Fields

机译:AAVSO星场中的可疑变量

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摘要

The master listing of stars observed by the AAVSO is listed in the"Validation File". The file lists commonly observed variable stars but alsolists many "obscure" stars within the fields of view that observers over theyears have suspected of being variable. Over the century-long history of theAAVSO over 1,200 such suspects have been added, but this population hasnever been investigated in detail. Our project first identified each suspect with acatalogue name and position, then using CCD cameras we are now sorting outthe true variables from non-variable stars. A small but significant percentageof these stars turn out to be variable, sometimes of surprisingly large range.Unfortunately, some of these variables have been used as comparison starsby visual observers over the years. And noW with the fields being explored byCCD camera users, even small-range unrecognized variables stars can causeconfusion and skewed data. It is thus important to identify the field suspectsand eliminate them as comparison stars.
机译:由“ AAVSO”观测到的恒星的主列表在“验证文件”中列出。该文件列出了通常观察到的变星,但也列出了多年来观察者怀疑是变星的视场中的许多“模糊”星。在AAVSO的长达一个世纪的历史中,已经添加了1200多名此类嫌疑犯,但从未对此人口进行过详细调查。我们的项目首先使用目录名称和位置来识别每个嫌疑犯,然后使用CCD摄像头从不可变恒星中筛选出真实变量。这些恒星中很小但占很大比例的恒星却是可变的,有时范围出乎意料。不幸的是,这些年来,其中一些变星已被视觉观察者用作比较恒星。现在,随着CCD相机用户正在探索的领域,即使是小范围的无法识别的恒星也会引起混乱和数据偏斜。因此,重要的是要识别现场嫌疑人,并消除它们作为比较星。

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