Cyclotron humps in AM HER systems. V - Two poles in DP Leo

Details Cyclotron humps in AM HER systems. V - Two poles in DP Leo Cyclotron humps in AM HER systems. V - Two poles in DP Leo

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.260..696c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 260, no. 3, p. 696-704.

Astronomy and Astrophysics

Astronomy

23

Cyclotron Radiation, Eclipsing Binary Stars, Stellar Magnetic Fields, Stellar Models, Light Curve, Linear Polarization, Stellar Mass Accretion, Stellar Orbits

Scientific paper

We have modelled phase-resolved spectroscopic data of DP Leo to explain the appearance of an unusually strongly peaked cyclotron hump at 6100 A. This can be modelled by emission from the second accretion region with almost twice the magnetic field of the main region (59 and 30.5 MG respectively). We show also that emission from such regions produces light and polarization curves which are consistent with observations.

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