Cyclotron radiation in UZ Fornacis (=EXO033319 - 2554.2) in a low state of accretion

Details Cyclotron radiation in UZ Fornacis (=EXO033319 - 2554.2) in a low state of accretion Cyclotron radiation in UZ Fornacis (=EXO033319 - 2554.2) in a low state of accretion

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...230..120s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 230, no. 1, April 1990, p. 120-126.

Astronomy and Astrophysics

Astrophysics

48

Cyclotron Radiation, Eclipsing Binary Stars, Stellar Mass Accretion, Magnetic Field Configurations, Stellar Magnetic Fields, Stellar Spectrophotometry, White Dwarf Stars

Scientific paper

A detailed analysis is presented of the cyclotron properties of UZ For in a state of low accretion. The results of low-resolution spectrophotometry are compared with theoretical models, and the main plasma parameters of the emission regions of UZ For are derived, including temperature, magnetic field strength, and the geometric size and location on the white dwarf. The cyclotron properties of a secondary emission region at the opposite pole are then discussed, and the results are compared with those of earlier studies.

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