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The light curve of V605 Aql

H. W. Duerbeck·M. L. Hazen·A. A. Misch·W. C. Seitter
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Abstract

``Nova Aquilae No. 4'', discovered in 1919, later renamed V605 Aql, was recognized to be a final helium flash object only in the 1980s. Clayton and De Marco (1997) gave a detailed description of the available spectroscopic and photometric material. Here we try to re-analyze the photometric record. The photographic material is still available and has been used to construct a revised light curve. Only fragments of the visual observations were published; the remainder appears to be lost.

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H. W. Duerbeck, M. L. Hazen, A. A. Misch, W. C. Seitter. 2001-02-20. The light curve of V605 Aql. https://arxiv.org/abs/astro-ph/0102347

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