The magnetically controlled stellar wind of HD 21699

Details The magnetically controlled stellar wind of HD 21699 The magnetically controlled stellar wind of HD 21699

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aj.....90.1354b&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 90, July 1985, p. 1354-1362. Research supported by the Research Corp. and University

Other

43

Magnetic Stars, Peculiar Stars, Stellar Magnetic Fields, Stellar Mass Ejection, Stellar Winds, Ultraviolet Spectra, Carbon, Iue, Line Spectra, Magnetic Variations, Polarimetry, Stellar Spectrophotometry, Zeeman Effect

Scientific paper

The authors report the discovery of a magnetically controlled stellar mass outflow in the helium-weak sn star HD 21699 = HR 1063. IUE observations show that the C IV resonance doublet is variable on the rotational time scale of about 2.5 days, and that there are no other observable spectrum variations in the UV. The magnetic field reverses sign on the rotational time scale. An interpretation of the observations in terms of magnetically structured jets is presented.

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