Insight into the OH polarimetric structure of OH 26.5+0.6

TL;DR

This study reveals the magnetic field structure in the OH shell of the star OH 26.5+0.6 using polarimetric interferometric observations, showing a poloidal magnetic field and a spheroidal outflow.

Contribution

First detailed polarimetric mapping of the magnetic field in the OH shell of OH 26.5+0.6, providing insights into its magnetic and outflow structure.

Findings

Magnetic field is poloidal and inclined 40-60° to the line of sight.

Maser spots show spheroidal distribution with filamentary structures.

Outer shell regions exhibit high linear polarisation up to 66%.

Abstract

We present the first view of the magnetic field structure in the OH shell of the extreme OH/IR star OH 26.5+0.6. MERLIN interferometric observations of this object were obtained in December 1993 in full polarisation, at 1612, 1665 and 1667 MHz. The maser spots show a spheroidal distribution both at 1612 and 1667 MHz, while at 1665 MHz emission from the blue-shifted maser peak is concentrated on the stellar position, and the red-shifted peak emission exhibits a filamentary structure oriented on a SE-NW axis. The linear polarisation in both main lines is rather faint, ranging from 9 to 20% at 1665 MHz and from 0 to 30% at 1667 MHz. At 1612 MHz most maser spots exhibit a similar range of linear polarisation although those in the outermost parts of the envelope reach values as high as 66%. This is particularly apparent in the southern part of the shell. The detailed distribution of the polarisation vectors could only be obtained at 1612 MHz. The polarisation vectors show a highly structured distribution indicative of a poloidal magnetic field inclined by 40-60$^\circ$ to the line of sight. The velocity distribution of the maser spots with respect to the radial distance is well explained by an isotropic outflow at constant velocity in the case of a prolate shaped spheroid envelope, also tilted about 45-65$^\circ$ to the line of sight.