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High latitude gas in the Beta Pictoris system. A possible origin related to Falling Evaporating Bodies | | Hervé Beust
; Pierre Valiron
; | | Date: |
9 Jan 2007 | | Abstract: | The presence of off-plane Ca II ions in the Beta Pictoris disk, and the non-detection of off-plane Na I atoms, can be explained as a consequence of the evaporation process of Falling Evaporating Bodies (FEBs). In the star-grazing regime, the FEBs are subject to inclination oscillations up to 30 - 40 degrees that causes most metallic species released by sublimation to move off plane The ions are be stopped at about 100 AU from the star. We show that collisions with a neutral medium can stop the ions. The required H I column density is reduced to 10^17 cm^-2, one order of magnitude below present detection limits. We also investigate the possibility that the ions are slowed down magnetically. While the sole action of a magnetic field of the order of 1 microGauss is not effective, the combined effect of magnetic and collisional deceleration processes lead to an additional lowering of the required H I column density. | | Source: | arXiv, astro-ph/0701241 | | Services: | Forum | Review | PDF | Favorites | |
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