Detection of an extremely strong magnetic field in the double-degenerate binary merger product HD 144941. Issue 1 (28th July 2021)

• Record Type: Journal Article
• Authors: Shultz, M E; Kochukhov, O; Labadie-Bartz, J; David-Uraz, A; Owocki, S P
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 507:Issue 1(2021)
• Page Start: 1283
• Page End: 1295
• Publication Date: 2021-07-28
• Subjects: stars: chemically peculiar -- circumstellar matter -- stars: early-type -- stars: individual: HD 144941 -- stars: magnetic field -- subdwarfs; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stab2162
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: HD 144941 is an extreme He (EHe) star, a rare class of subdwarf OB star formed from the merger of two white dwarf (WD) stars. Uniquely amongst EHe stars, its light curve has been reported to be modulated entirely by rotation, suggesting the presence of a magnetic field. Here, we report the first high-resolution spectropolarimetric observations of HD 144941, in which we detect an extremely strong magnetic field both in circular polarization (with a line-of-sight magnetic field averaged over the stellar disc 〈 Bz 〉 ∼−8 kG) and in Zeeman splitting of spectral lines (yielding a magnetic modulus of 〈 B 〉 ∼17 kG). We also report for the first time weak H α emission consistent with an origin and a centrifugal magnetosphere. HD 144941's atmospheric parameters could be consistent with either a subdwarf or a main-sequence (MS) star, and its surface abundances are neither similar to other EHe stars nor to He-strong magnetic stars. However, its H α emission properties can only be reproduced if its mass is around 1 M⊙, indicating that it must be a post-MS object. Since there is no indication of binarity, it is unlikely to be a stripped star, and was therefore most likely produced in a WD merger. HD 144941 is therefore further evidence that mergers are a viable pathway for the generation of fossil magnetic fields.