DETECTION OF CYCLOTRON LINES IN BL HYI
Citation
L. Ferrario et al., DETECTION OF CYCLOTRON LINES IN BL HYI, Publications of the Astronomical Society of Australia, 12(1), 1995, pp. 81-83
Categorie Soggetti
Astronomy & Astrophysics
SICI code
1323-3580(1995)12:1<81:DOCLIB>2.0.ZU;2-S
Abstract
We present near-infrared spectroscopic observations over the wavelengt
h range 0.9 to 2.5 mu m 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 mu m. We have interpreted these featu
res as arising from a cyclotron emission region located near the white
dwarf's polar cap of magnetic field strength B-p = 23 MG.