Accretion discs, jets and high energy phenomena in by Jean Heyvaerts (auth.), Vassily Beskin, Gilles Henri,

By Jean Heyvaerts (auth.), Vassily Beskin, Gilles Henri, François Menard, Guy Pelletier, Jean Dalibard (eds.)

The accretion method is assumed to play a key function within the Universe. This e-book explains, in a kind intelligible to graduate scholars, its relation to the formation of latest stars, to the power unlock in compact items and to the formation of black holes. The monograph describes how accretion strategies are with regards to the presence of jets in stellar gadgets and lively galactic nuclei and to jet formation. The authors deal with theoretical paintings in addition to present observational evidence. This quantity of the hugely esteemed Les Houches sequence is intended as a complicated textual content which can serve to draw scholars to intriguing new examine paintings in astrophysics.

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Additional info for Accretion discs, jets and high energy phenomena in astrophysics: Les Houches Session LXXVIII, 29 July-23 August, 2002

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4). 43) must vanish. Any failure J. Heyvaerts: Accretion and Ejection-Related MHD 51 to satisfy this Alfv´en regularity condition is punished by obtaining a solution in which magnetic and flow surfaces have a kink at their crossing of the Alfv´en surface. This kink represents a rotational discontinuity standing in the flow. 44) gA (r, z, a, ∇a) = 0 at the Alfv´en surface. An explicit form of it has been derived in [13]. 45) The coefficients A, B and C may be functions of x, y, f and its first order derivatives.

Using this remark, it can be shown that the flaring magnetic surfaces are asymptotically conical when the wind subtends a finite magnetic flux [14, 15]. 16) implies that at large distances no current flows between flaring magnetic surfaces. For non-zero total current this implies that the current that they enclose flows in some region about the polar axis, where the magnetic surfaces are cylindrical. Paraboloidal magnetic surfaces do not enclose a finite current asymptotically, unless the magnetic flux subtending the wind source is infinite [14].

3) between its pressure and its density. 6) E + v × B = 0. 7) The gravitational field derives from an axisymmetrical gravitational potential Φg (r, z). Self-gravity of the wind is neglected. 6). 4) the electric field is electrostatic and given by E = −∇Φe (r, z). 2, that Φe is a surface function: Φe (r, z) = Φe (a(r, z)) = Φe (a). 9) From Φe (a) we define a rotation rate Ω(a), by no means equal to vθ /r, by Ω(a) = dΦe /da. 9) into account. Its azimuthal part reduces to (v P × B P ) = 0, which can also be written as ρv P = α(r, z)B P .

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