Magnetic fields and nuclear reactions at stellar surfaces

Details Magnetic fields and nuclear reactions at stellar surfaces Magnetic fields and nuclear reactions at stellar surfaces

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izssr..43..872d&link_type=abstract

(Seminar po Iadernoi Kosmicheskoi Fizike, 10th, Leningrad, USSR, Oct. 1978.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia

Astronomy and Astrophysics

Astrophysics

Novae, Nuclear Reactions, Stellar Magnetic Fields, White Dwarf Stars, Nuclear Astrophysics, Perturbation, Stellar Temperature

Scientific paper

The origin of strong magnetic fields on the white-dwarf components of nova systems and evidence for the existence of such strong magnetic fields are considered. Magnetic-field generation due to temperature perturbations or some other perturbations of the white-dwarf parameters is analyzed, and it is shown that the development of such an instability can give rise to magnetic fields in excess of 1 million to 10 million gauss. Other possible magnetic-field generation mechanisms are also examined.

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