Magnetic fields in AM HER systems - A possible field for 1E1048.5 + 5241 (EK UMa) from cyclotron humps

Details Magnetic fields in AM HER systems - A possible field for 1E1048.5 + 5241 (EK UMa) from cyclotron humps Magnetic fields in AM HER systems - A possible field for 1E1048.5 + 5241 (EK UMa) from cyclotron humps

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.243..565c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 243, April 15, 1990, p. 565-569. Research supported by

Astronomy and Astrophysics

Astronomy

12

Cataclysmic Variables, Cyclotron Radiation, Interstellar Magnetic Fields, Stellar Mass Accretion, White Dwarf Stars, Infrared Spectra, Mass Transfer, X Ray Spectra

Scientific paper

Cyclotron humps have been detected in the spectrum of the 19th mag AM Her system IE1048.5 + 5241 at certain phases. Two methods of determining the magnetic field were used; these, with information from the spectral slope, both yield a magnetic field strength of 47 MG. The temperature in the emitting region is less well determined but is likely to be higher than 10 keV.

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