Asymptotic Self-Similarity in Magnetized Winds from Stars and Disks

Details Asymptotic Self-Similarity in Magnetized Winds from Stars and Disks Asymptotic Self-Similarity in Magnetized Winds from Stars and Disks

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.8102s&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #81.02; Bulletin of the American Astronomical Society, Vol. 25, p.1419

Astronomy and Astrophysics

Astronomy

Scientific paper

Magnetized winds emerging from rapidly rotating stars and disks may self-collimate at large distances from their sources. Self-similar models of magnetized winds (Blandford and Payne 1982) reflect this property. However, the solutions to general problem of magnetized wind flow do not in general exhibit global self-similarity. However, we discuss the asymptotic approach to self-similarity of magnetized winds.

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