https://doi.org/10.1051/epjconf/202024005001
On the origin of high Doppler velocity wings in the spectra of O-rich AGB stars
Department of Astrophysics, Vietnam National Space Center, Vietnam Academy of Sciences and Technologies (VNSC/VAST), 18 Hoang Quoc Viet, Nghia Do, Cau Giay, Hanoi, Vietnam
1 Corresponding author: dthoai@vnsc.org.vn
Published online: 21 August 2020
Millimetre ALMA observations of the nascent winds of several Oxygen rich AGB stars have revealed the high Doppler velocity wings in their spectra. However, the physics underlying their production is unclear. In this paper, we illustrate the argument with four examples of oxygen-rich AGB stars: EP Aqr, R Dor, L2 Pup and Mira Ceti.
© The Authors, published by EDP Sciences, 2020
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
