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..343b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 148, no. 2, Oct. 1988, p. 343-361.

Astronomy and Astrophysics

Astrophysics

10

Early Stars, Jet Flow, Leptons, Star Formation, Stellar Models, Accretion Disks, Molecular Clouds, Pair Production, Stellar Rotation, Stellar Winds

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 the e± pair-formation threshold (of 1012eV). Pair-plasma jets are thought to be centrifugally driven by young stars during their first 104±1years of rapid rotation.

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