High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The
PANORAMA survey
High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The
PANORAMA survey
As mass-losing asymptotic giant branch (AGB) stars evolve to planetary nebulae (PNe), the mass outflow geometries transform from nearly spherical to extreme aspherical. The physical mechanisms governing this transformation are widely believed to be linked to binarity and the associated production of disks and fast jets during transitional (post-AGB) evolutionary …