7.4. GALAXIES 455
Jet
Accretion
(a) (b)
Accretion
Jet
Jet
Figure 7.11: (a) A jet in the latitudinal circulation withk=1 cell, two jets in the latitudinal
circulation withk=2 cells.
the bifurcated solution of (7.4.26), which can be expressed as
Pr=R^2 sQr,
whereQris independent ofRs. Thus, the radial force (7.4.35) nearr=Rsis approximatively
written as
(7.4.37) fr=
ν
1 −Rs/r
QRs, r=Rs+ ̃r for 0< ̃r≪Rs.
LetfEbe the lower limit of the effective force, which is defined as that the total radial
forceFrin the third equation of (7.4.26) is positive providedfr>fE:
Fr>0 if fr>fE.
LetREbe the effective distance:
fr>fE if Rs<r<Rs+RE.
Then, it follows from (7.4.37) that
(7.4.38) RE=kRs (k=νQRs/fE).
It is clear that there is a critical distanceRcsuch that
(7.4.39)
a jet forms ifRE>Rc orRs>k−^1 Rc,
no jet forms ifRE<Rc orRs<k−^1 Rc.
The criterion (7.4.39) is the condition for jet generation.
The condition (7.4.39) can be equivalently rewritten as that there is a critical massMc
such that the galactic nucleus is active if its massMis bigger thanMc, i.e. M>Mc. By
(7.4.21), we have
105 M⊙<Mc or 106 M⊙<Mc.