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Stars Classified as Constant in the General Catalogue of Variable Stars, II

机译:在变星总目录中被分类为常数的星,II

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摘要

Photometric observations have been made of 36 stars classified as CST or CST: in the General Catalogue of Variable Stars. Six of these stars are found to vary and three others were deemed possible variables. Of the certain variables, two (MR Her and TY Sge) are red pulsators, one (V1585 Cyg) is a rapid irregular variable, one is apparently a short period Cepheid-strip star (V432 Oph), one is an eclipsing binary (AQ Boo), and one is of uncertain type (V351 Cyg). The stars we have observed as MR Her and TY Sge are the same ones which were identified on finding charts in the discovery papers, suggesting that these stars have intervals of variability and intervals of quiescence. V432 Oph is of special interest because our photometry indicates that it may be either a double mode Cepheid or a peculiar long-period RR Lyrae star depending on which of a couple of possible periods turns out to be correct.
机译:在变星总目录中,对36颗分类为CST或CST的恒星进行了光度观测。发现其中六颗恒星在变化,另外三颗被认为是可能的变量。在某些变量中,两个(MR Her和TY Sge)是红色波轮,一个(V1585 Cyg)是快速不规则变量,一个显然是短时造父变星(V432 Oph),一个是日蚀双星(AQ) Boo),其中之一是不确定类型(V351 Cyg)。我们观察到的恒星MR Her和TY Sge与发现论文中发现图表时发现的恒星相同,这表明这些恒星具有变异性间隔和静止性间隔。 V432 Oph特别令人关注,因为我们的测光表明它可能是双模式造父变星,也可能是奇特的长周期RR天琴星,具体取决于几个可能的周期中的哪个是正确的。

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  • 作者

    Schmidt, Edward G.;

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  • 年度 1996
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