An MHD-driven Disk Wind Outflow in SDSS J0300+0048?

Simple item page
dc.creatorHall, Patrick B.
dc.creatorHutsemekers, Damien
dc.date2003-11-25
dc.date.accessioned2026-07-07T02:11:20Z
dc.date.available2026-07-07T02:11:20Z
dc.descriptionThe outflow in SDSS J030000.56+004828.0 has the highest low-ionization metal-line column density yet reported for a broad absorption line quasar. The absorption from different ions is also segregated as a function of velocity in a way that can only be explained by a disk wind outflow. Furthermore, the presence of the such large column densities of gas at the high observed outflow velocities may be incompatible with purely radiative acceleration. MHD contributions to the acceleration should be considered seriously.
dc.descriptionto appear in AGN Physics with the Sloan Digital Sky Survey, ed. G. T. Richards and P. B. Hall
dc.identifierhttps://arxiv.org/abs/astro-ph/0311561
dc.identifierhttp://arxiv.org/abs/astro-ph/0311561
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7046
dc.subjectAstrophysics
dc.titleAn MHD-driven Disk Wind Outflow in SDSS J0300+0048?
dc.typetext

Files

Collections

arXiv