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Optical Observations of FY Persei

Published online by Cambridge University Press:  12 April 2016

Akira Okazaki
Akira Okazaki*
Affiliation:
Department of Science Education, Gunma University, Maebashi, Japan

Abstract

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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.

Type
II. Observational Facts
Information
International Astronomical Union Colloquium , Volume 134: Nonlinear Phenomena in Stellar Variability , 1993 , pp. 227 - 229
Copyright
Copyright © Kluwer 1993

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