Multi-line diagnostics of the axi-symmetric wind around the MS-type AGB star RS Cancri
1 IRAM, 300 rue de la Piscine, 38406 St. Martin d’Hères, France
2 LERMA, Observatoire de Paris, 61 av. de l’Observatoire, 75014 Paris, France
3 VNSC, VAST, 18 Hoang Quoc Viet, Cau Giay, Ha Noi, Viet Nam
4 LPENS, 24 rue Lhomond, 75231 Paris, France
5 I. Physikalisches Institut, Uni Köln, Zülpicher Str. 77, 50937 Köln, Germany
* e-mail: firstname.lastname@example.org
Published online: 7 September 2022
We present data recently obtained with NOEMA/PolyFiX on the MS-type Asymptotic Giant Branch (AGB) star RS Cnc, allowing to characterize in detail the structure of its wind. These results became possible by the recent advances of the NOEMA observatory, which combine large spectral bandwidth with high sensitivity together with still increasing spatial resolution.
© The Authors, Published by EDP Sciences, 2022
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).