Multi-band ALMA Polarization Observations of BHB07-11 Reveal Aligned Dust Grains in Complex Spiral Arm Structures
Austen Fourkas, Leslie W. Looney, Zhe-Yu Daniel Lin, Martin Radecki, Zhi-Yun Li, John J. Tobin, Ian W. Stephens, Manuel Fern\'andez-L\'opez, Haifeng Yang, Woojin Kwon, Rachel Harrison

TL;DR
This study uses multi-band ALMA polarization observations of BHB07-11 to demonstrate that dust grains in its spiral arms are aligned via a velocity flow mechanism rather than magnetic fields, revealing insights into grain alignment processes.
Contribution
It provides the first evidence supporting a velocity flow alignment mechanism for dust grains in a complex circumstellar disk with spiral structures.
Findings
Polarization vectors follow spiral arm structures across multiple bands.
Alignment mechanism is consistent with velocity flow, not magnetic fields.
Supports the badminton birdie-like alignment model in circumstellar environments.
Abstract
Polarization-mode observations from the Atacama Large Millimeter/submillimeter Array (ALMA) are powerful tools for studying the dust grain populations in circumstellar disks. Many sources exhibit polarization signatures consistent with aligned dust grains, yet the physical origin of this alignment remains uncertain. One such source is BHB07-11, a Class I protobinary object in the Pipe Nebula with complex spiral arm structures in its circumbinary disk. While magnetic fields are often invoked to explain grain alignment in the interstellar medium, the contrasting conditions in circumstellar disk environments demand further investigation into grain alignment mechanisms. To determine BHB07-11's dominant polarization mechanism, we leverage ALMA polarization-mode dust continuum observations in Bands 3 (=3.1 mm), 6 (=1.3 mm), and 7 (=0.87 mm), in combination with…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
