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Novae and Related Stars pp 179Cite as

Multi-Band Photometry of Nova Cygni 1975

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 65))

Abstract

Infrared and optical photometries of Nova Cygni 1975 were carried out from 1975 September 2, immediately after the light maximum, until November 10, the 69th day after the maximum.

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Author information

Authors and Affiliations

  1. Department of Physics, Kyoto University, Kyoto, Japan

    K. Kawara, T. Maihara, K. Noguchi, N. Oda, H. Okuda & S. Sato

  2. Astronomical Institute, Tohoku University, Sendai, Japan

    M. Oishi

  3. Department of Physics, Nagoya University, Nagoya, Japan

    T. Iijima

Authors
  1. K. Kawara
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  2. T. Maihara
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  3. K. Noguchi
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  4. N. Oda
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  5. H. Okuda
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  6. S. Sato
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  7. M. Oishi
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  8. T. Iijima
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Editor information

Editors and Affiliations

  1. Institut d’Astrophysique, Paris, France

    M. Friedjung

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Copyright information

© 1977 D. Reidel Publishing Company, Dordrecht, Holland

About this paper

Cite this paper

Kawara, K. et al. (1977). Multi-Band 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_37

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  • DOI: https://doi.org/10.1007/978-94-010-1217-1_37

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-1219-5

  • Online ISBN: 978-94-010-1217-1

  • eBook Packages: Springer Book Archive

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