Polarization Substructure in the Spiral-dominated HH 111 Disk: Evidence for Grain Growth

The HH 111 protostellar disk has recently been found to host a pair of spiral arms. Here we report the dust polarization results in the disk as well as the inner envelope around it, obtained with the Atacama Large Millimeter/submillimeter Array in continuum at λ ∼ 870 μ m and ∼0.″05 resolution. In t...

ver descrição completa

Detalhes bibliográficos

Principais autores:	Chin-Fei Lee, Zhi-Yun Li, Tao-Chung Ching, Haifeng Yang, Shih-Ping Lai, Zhe-Yu Daniel Lin, Ying-Chi Hu
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2024-01-01
coleção:	The Astrophysical Journal Letters
Assuntos:	Star formation Stellar accretion disks Polarimetry Magnetic fields
Acesso em linha:	https://doi.org/10.3847/2041-8213/ad68e1
Tags:	Adicionar Tag Sem tags, seja o primeiro a adicionar uma tag!