Discovery of polarizations from ground state absorption lines: tracer of sub-Gauss magnetic field on 89Her
arXiv:1903.08675 · doi:10.3847/2041-8213/abb8e1
Abstract
We report the identification of the polarization of ground state absorption lines from post-AGB 89~Hercules. Two ground state neutral iron lines are found to have counterintuitive high-amplitude polarizations and an unchanged polarization direction through the orbital period, as opposed to the pattern of polarizations of absorption lines from excited states, which are synchronized with the orbital phase owing to optical pumping. This can be explained with magnetic realignment on the ground state. The 3D mean magnetic field is thereby unveiled from the degree and direction of the polarizations of the two iron lines. The field strength is also constrained to be . Our result has thus improved the accuracy by orders of magnitude compared to the previous upper limit set by non-detection of the Zeeman effect.
arXiv comment7 pages, 4 figures, ApJ Lett. accepted
References in corpus (11)
- The nebula around the post-AGB star 89 Her
- Polarization of absorption lines as a diagnostics of circumstellar, interstellar and intergalactic magnetic fields: Fine structure atoms
- First detection of surface magnetic fields in Post-AGB stars : the cases of U Monocerotis and R Scuti
- Atomic alignment and Diagnostics of Magnetic Fields in Diffuse Media
- Polarization from aligned atoms as a diagnostics of circumstellar, AGN and interstellar magnetic fields: II. Atoms with Hyperfine Structure
- Tracing Magnetic Fields with Ground State Alignment
- Polarisation of submillimetre lines from interstellar medium
- Multi-band polarimetry of post-asymptotic giant branch stars stars. Optical measurements
- Tracing Magnetic Fields by Atomic Alignment in Extended Radiation Fields
- Study of Interplanetary Magnetic Field with Ground State Alignment
- The solar-like "Second Spectrum" and the polarised metal lines in emission of the post-AGB binary 89 Herculis
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