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The CHARA Array Polarization Model and Prospects for Spectropolarimetry

Polarimetric data provide key insights into infrared emission mechanisms in the inner disks of young stellar objects (YSOs) and the details of dust formation around asymptotic giant branch (AGB) stars. While polarization measurements are well-established in radio interferometry, they remain challeng...

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Furkejuvvon:
Váldodahkkit: Linling Shuai, John D. Monnier, Benjamin R. Setterholm, Stefan Kraus, Narsireddy Anugu, Tyler Gardner, Jean-Baptiste Le Bouquin, Gail H. Schaefer
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: IOP Publishing 2025-01-01
Ráidu:The Astronomical Journal
Fáttát:
Optical interferometry
Spectropolarimetry
Circumstellar dust
Liŋkkat:https://doi.org/10.3847/1538-3881/ae0648
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