2010PASP..122.1334P

Query : 2010PASP..122.1334P

2010PASP..122.1334P - Publ. Astron. Soc. Pac., 122, 1334-1340 (2010/November-0)

A magnetohydrodynamic model for the AGB star: preplanetary nebula symbiosis.

PASCOLI G. and LAHOCHE L.

Abstract (from CDS):

In this article, a magnetohydrodynamic (MHD) model is presented that is aimed at understanding the anisotropic mass loss by an AGB star and subsequent bipolar planetary nebula formation. The main challenge in developing such a model was to simultaneously treat the dynamo engine in the core region of the AGB progenitor, magnetic buoyancy, meridional circulation, and gas ejection in a self-consistent manner. A previous article did not incorporate the dynamo and the feedback of the produced magnetic field on differential rotation.

Abstract Copyright: ∼

Journal keyword(s): ISM

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 THA 35-II-27 PN 10 19 32.501 -60 13 29.48     12.5     B:Ie 90 0
2 PN M 2-9 PN 17 05 37.96152 -10 08 32.5068           ~ 532 0
3 NGC 6543 PN 17 58 33.4039587288 +66 37 58.750734000   11.09 11.28     [WC] 1197 2
4 PN Fg 3 PN 18 00 11.8162949280 -38 49 52.619928204   12.80 11.18     ~ 101 1

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