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A Photometric Investigation of the Magnetic Star 53 Cameloprdalis

Published online by Cambridge University Press:  12 April 2016

M. Muciek ,
P. North ,
F. Rufener  and
J. Gertner
M. Muciek
Affiliation:
Institute of Astronomy, Nicolaus Copernicus Universityul. Chopina 12/18, PL 87100 Torún, Poland
P. North
Affiliation:
Institut d’Astronomie de l’Université de LausanneCH-1290 Chavannes-des-Bois, Switzerland
F. Rufener
Affiliation:
Observatoire de Genève, CH-1290 Sauverny, Switzerland
J. Gertner
Affiliation:
Institute of Astronomy, Nicolaus Copernicus Universityul. Chopina 12/18, PL 87100 Torún, Poland

Abstract

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Geneva photometry of the important and relatively well known Ap star 53 Cam (HR 3109, HD 65339) is presented. These 27 data, which cover rather evenly the rotational phase interval, are compared with the photometric data in ten bandpasses published by Musielok et al. (1980). They allow to show that at least four “null-wavelength regions” occur between 3400 and 7800 Å.

Type
Section II - Systematics, Photometry
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 199
Copyright
Copyright © Reidel 1986

References

Borra, E.F., Landstreet, J.D: 1977, Astrophys. J. 212, 141 CrossRefGoogle Scholar
Musielok, B., Lange, D., Schöneich, W., Hildebrandt, G., Zhelvanova, E., Hempelmann, A., Salmanov, G.: 1980, Astr. Nachr. 301, 71 CrossRefGoogle Scholar