Early F-type "variables without a cause"

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Scientific paper

Three years ago in this newsletter (Krisciunas 1990) I presented some information on the odd variable star 9 Aurigae, an otherwise normal F0 V star. Its V-band brightness has a range of nearly 0. 1 magnitude. I should point out that the graph given in that note is wrong. No period shorter than an hour has been confirmed on the basis of more extensive and more accurate photometry.

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