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Optical observations of FY Persei

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Abstract

The results are presented of multi-channel photometry and spectroscopy of the suspected nova-like variable FY Per. These results suggest that FY Per may be a Herbig Ae/Be star rather than a nova-like variable.

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Authors and Affiliations

  1. Department of Science Education, Gunma University, Maebashi, Japan

    Akira Okazaki

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  1. Akira Okazaki
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Okazaki, A. Optical observations of FY Persei. Astrophys Space Sci 210, 227–229 (1993). https://doi.org/10.1007/BF00657905

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  • DOI: https://doi.org/10.1007/BF00657905

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