Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-09-26
Mon.Not.Roy.Astron.Soc.376:599-608,2007
Astronomy and Astrophysics
Astrophysics
25 pages, 7 figures, submitted to MNRAS; revised to fix Fig. 5
Scientific paper
10.1111/j.1365-2966.2007.11417.x
The origin, evolution and role of magnetic fields in the production and shaping of proto-planetary and planetary nebulae (PPNe, PNe) is a subject of active research. Most PNe and PPNe are axisymmetric with many exhibiting highly collimated outflows, however, it is important to understand whether such structures can be generated by isolated stars or require the presence of a binary companion. Toward this end we study a dynamical, large-scale alpha-Omega interface dynamo operating in a 3.0 M_sun Asymptotic Giant Branch star (AGB) in both an isolated setting and one in which a low-mass companion is embedded inside the envelope. The back reaction of the fields on the shear is included and differential rotation and rotation deplete via turbulent dissipation and Poynting flux. For the isolated star, the shear must be resupplied in order to sufficiently sustain the dynamo. Furthermore, we investigate the energy requirements that convection must satisfy to accomplish this by analogy to the sun. For the common envelope case, a robust dynamo results, unbinding the envelope under a broad range of conditions. Two qualitatively different types of explosion may arise: (i) magnetically dominated, possibly resulting in collimated bipolar outflows and (ii) thermally induced from turbulent dissipation, possibly resulting in quasi-spherical outflows. A range of models is presented for a variety of companion masses.
Blackman Eric G.
Frank Alejandro
Nordhaus Jason
No associations
LandOfFree
Isolated vs. Common Envelope Dynamos in Planetary Nebula Progenitors does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Isolated vs. Common Envelope Dynamos in Planetary Nebula Progenitors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Isolated vs. Common Envelope Dynamos in Planetary Nebula Progenitors will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-166416