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Cambridge University Press (CUP), Publications of the Astronomical Society of Australia, 1(12), p. 81-83, 1995

DOI: 10.1017/s1323358000020087

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Detection of Cyclotron Lines in BL Hyi

Journal article published in 1995 by Lilia Ferrario, Dayal T. Wickramasinghe, Jeremy Bailey
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

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Postprint: archiving allowed
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Data provided by SHERPA/RoMEO

Abstract

AbstractWe present near-infrared spectroscopic observations over the wavelength range 0·9 to 2·5 μm of the AM Herculis system BL Hyi. During these observations, broad and resolvable cyclotron emission harmonics were visible near 1·25, 1·60 and 2·20 μm. We have interpreted these features as arising from a cyclotron emission region located near the white dwarf’s polar cap of magnetic field strength Bp = 23 MG.

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