Dynamical Properties of a Centrifugally Driven Outflow From a Disc Near a Black Hole

Details Dynamical Properties of a Centrifugally Driven Outflow From a Disc Near a Black Hole Dynamical Properties of a Centrifugally Driven Outflow From a Disc Near a Black Hole

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.226..165c&link_type=abstract

Astrophysics and Space Science, Volume 226, Issue 1, pp.165-168

Astronomy and Astrophysics

Astrophysics

1

Accretion Disk, Outflows, Black Holes

Scientific paper

The inclination of the field lines at the surface of the disc plays a crucial role on the nature of the magnetically driven flows. For the non-relativistic case, a centrifugally driven outflow of matter from the disc is possible, if the poloidal component of the magnetic field makes an angle of less than a critical 60° with the disc surface (Blandford and Payne 1982). We investigate the dynamical properties of the magnetically driven flows from the disc near a non-rotating black hole and find that the critical angle becomes larger than 60° when the flows start from the region near the black hole.

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