Photometric Observations of Nova Cygni 1986 = V1819-CYGNI

Astronomy and Astrophysics – Astronomy

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Scientific paper

The photoelectric UBVRI photometry of Nova Cygni 1986 during 1986
October to 1987 January is reported. The IR excess detected on December
1 and January 9 was more than in August-September. It is probably due to
the formation of the dust shell.

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