On the fastness parameter and the inner disc radius

Details On the fastness parameter and the inner disc radius On the fastness parameter and the inner disc radius

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.286l..25l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 286, Issue 2, pp. L25-L28.

Astronomy and Astrophysics

Astronomy

13

Accretion, Accretion Discs: Magnetic Fields

Scientific paper

Recently we proposed that gas funnelled by magnetic field lines from an accretion disc on to a magnetized compact star does not exert a significant material torque on the star. We show that a consequence of this result is that in rotational equilibrium the true inner disc radius is significantly smaller than the corotation radius (pi_inpi_co~=0.10-0.74).

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