Leptonic jets from young stellar objects?

Details Leptonic jets from young stellar objects? Leptonic jets from young stellar objects?

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.148..343j&link_type=abstract

Astrophysics and Space Science, Volume 148, Issue 2, pp.343-361

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Various explanations of the bipolar-flow phenomenon in star-forming regions are compared and confronted with the observed facts. It is concluded that stellar-wind interpretations are inconsistent with the constraints. The ‘exotic’ property of young stellar objects may be their extreme spin which implies strong magnetic fields and vacuum discharges above thee ± pair-formation threshold (of 1012 eV). Pair-plasma jets are thought to be centrifugally driven by young stars during their first 104±1 years of rapid rotation.

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