Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8917838c&link_type=abstract
Unknown
Astronomy and Astrophysics
Astronomy
Adiabatic Flow, Mach Number, Shock Waves, Accretion Disks, Black Holes (Astronomy), Transonic Flow
Scientific paper
We show that there is a lower limit of the shock strength Sigma = M(sub
-)/M(sub +), where M(sub -) and M(sub +) are the Mach numbers before and
after the shock, for adiabatic flows in vertical equilibrium. The limit
is independent of the nature of the force field governing the flow or
the mass flux and only depends upon the adiabatic index.
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