The light curve of V605 Aql

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dc.creatorDuerbeck, H. W.
dc.creatorHazen, M. L.
dc.creatorMisch, A. A.
dc.creatorSeitter, W. C.
dc.date2001-02-20
dc.date.accessioned2026-07-07T01:57:45Z
dc.date.available2026-07-07T01:57:45Z
dc.description``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.
dc.descriptionLaTeX, 6 pages, 1 ps-figure, to be published in ApSS
dc.identifierhttps://arxiv.org/abs/astro-ph/0102347
dc.identifierhttp://arxiv.org/abs/astro-ph/0102347
dc.identifierAstrophys.Space Sci. 279 (2002) 183-186
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2514
dc.subjectAstrophysics
dc.titleThe light curve of V605 Aql
dc.typetext

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