Abstract
Nova Cygni was observed 28 times at 100 days after visual maximum with the ultraviolet experiment on board the Astronomical Netherlands Satellite. The instrument is a 5-channel intermediate band (100–200 A) spectrophotometer. Central wavelengths for the channels are 1550, 1800, 2200, 2500 and 3300 A.
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© 1977 D. Reidel Publishing Company, Dordrecht, Holland
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Wu, CC. (1977). Ultraviolet Photometry of Nova Cygni 1975. In: Friedjung, M. (eds) Novae and Related Stars. Astrophysics and Space Science Library, vol 65. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1217-1_42
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DOI: https://doi.org/10.1007/978-94-010-1217-1_42
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