A boundary layer origin for bipolar flows

Details A boundary layer origin for bipolar flows A boundary layer origin for bipolar flows

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.236..107p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 236, Jan. 1, 1989, p. 107-115.

Astronomy and Astrophysics

Astronomy

69

Accretion Disks, Protostars, Stellar Winds, Boundary Layers, Stellar Magnetic Fields, Stellar Mass Accretion

Scientific paper

Consideration is given to the origin of the energetic winds which are seen to emanate from young stellar objects. It is argued that the most likely origin for such winds is in the boundary layer of the accretion disc which surrounds them, and that the driving is due to strong toroidal magnetic fields produced by the strong shear in the boundary layer region.

Affiliated with

Also associated with

No associations

Rating

A boundary layer origin for bipolar flows does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A boundary layer origin for bipolar flows, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A boundary layer origin for bipolar flows will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-828037