2017
DOI: 10.1017/s1743921317011486
View full text
|
|

Abstract: The full theory of polarized SiO maser emission from the near-circumstellar environment of Asymptotic Giant Branch stars has been the subject of debate, with theories ranging from classical Zeeman origins to predominantly non-Zeeman anisotropic excitation or propagation effects. Features with an internal electric vector position angle (EVPA) rotation of ∼ π/2 offer unique constraints on theoretical models. In this work, results are presented for one such feature that persisted across five epochs of SiO ν = 1,… Show more

Help me understand this page
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

0
0
0
0
0

Citation Types

0
0
0

Publication Types

Select...

Relationship

0
0

Authors

Journals