Photometry, Spectroscopy, and Classification of Nova V475 Scuti

Details Photometry, Spectroscopy, and Classification of Nova V475 Scuti Photometry, Spectroscopy, and Classification of Nova V475 Scuti

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005javso..34...36s&link_type=abstract

The Journal of the American Association of Variable Star Observers, Vol 34, No. 1, p. 36-42

Physics

V475 Sct, Photometry, Spectroscopy

Scientific paper

The classification of and distance to the nova V475 Scuti are
determined. This paper reports that the nova type for V475 Sct is
determined to be a slow Fe II nova at a distance of 2 ± 0.6 kpc
(approximately 6500 ly).

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