Multi-line diagnostics of the axi-symmetric wind around the MS-type AGB star RS Cancri - Observatoire de Paris Accéder directement au contenu
Communication Dans Un Congrès Année : 2022

Multi-line diagnostics of the axi-symmetric wind around the MS-type AGB star RS Cancri

Résumé

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.

Dates et versions

obspm-03992955 , version 1 (16-02-2023)

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Citer

Jan Martin Winters, Thibaut Le Bertre, Do Thi Hoai, Ka Tat Wong, Pham Tuyet Nhung, et al.. Multi-line diagnostics of the axi-symmetric wind around the MS-type AGB star RS Cancri. Multi-line Diagnostics of the Interstellar Medium, Apr 2022, Nice, France. pp.00030, ⟨10.1051/epjconf/202226500030⟩. ⟨obspm-03992955⟩
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