The light curve of V605 Aql
Astrophysics
2007-05-23 v1
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.
Keywords
Cite
@article{arxiv.astro-ph/0102347,
title = {The light curve of V605 Aql},
author = {H. W. Duerbeck and M. L. Hazen and A. A. Misch and W. C. Seitter},
journal= {arXiv preprint arXiv:astro-ph/0102347},
year = {2007}
}
Comments
LaTeX, 6 pages, 1 ps-figure, to be published in ApSS