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Cited article:

ATOMIUM: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae - I. Morpho-kinematical interpretation of CO and SiO emission

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Stellar Evolution Along the Asymptotic Giant Branch as Revealed by the Shape of Miras’ Visual Light Curves

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The Astrophysical Journal 982 (2) 201 (2025)
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ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA

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Chemical tracers of a highly eccentric AGB–main-sequence star binary

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Stellar Evolution in Real Time. II. R Hydrae and an Open-Source Grid of >3000 Seismic TP-AGB Models Computed with MESA

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The impact of third dredge-up on the mass loss of Mira variables

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ATOMIUM: Probing the inner wind of evolved O-rich stars with new, highly excited H2O and OH lines

A. Baudry, K. T. Wong, S. Etoka, et al.
Astronomy & Astrophysics 674 A125 (2023)
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Contributions of Rotation, Expansion and Line Broadening to the Morphology and Kinematics of the Inner CSE of Oxygen-rich AGB Star R Hya

Pham Tuyet Nhung, Do Thi Hoai, Pierre Darriulat, et al.
Research in Astronomy and Astrophysics 23 (1) 015004 (2023)
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ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars

C. A. Gottlieb, L. Decin, A. M. S. Richards, et al.
Astronomy & Astrophysics 660 A94 (2022)
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SPH modelling of companion-perturbed AGB outflows including a new morphology classification scheme

S. Maes, W. Homan, J. Malfait, et al.
Astronomy & Astrophysics 653 A25 (2021)
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