Author:
Darriulat Pierre,Hoai Do Thi,Nhung Pham Thi Tuyet,Diep Pham Ngoc,Ngoc Nguyen Bich,Thai Tran Thi,Anh Pham Tuan
Publisher
Cellule MathDoc/Centre Mersenne
Reference142 articles.
1. Global 3D radiation-hydrodynamics models of AGB stars; Effects of convection and radial pulsations on atmospheric structures;Freytag, B.;Astron. Astrophys.,2017
2. Mass loss of stars on the asymptotic giant branch; Mechanisms, models and measurements;Höfner, S.;Astron. Astrophys.,2018
3. Exploring the origin of clumpy dust clouds around cool giants; A global 3D RHD model of a dust-forming M-type AGB star;Höfner, S.;Astron. Astrophys.,2019
4. Global 3D radiation-hydrodynamical models of AGB stars with dust-driven winds;Freytag, B.;Astron. Astrophys.,2023
5. Study of the aluminium content in AGB winds using ALMA. Indications for the presence of gas-phase (AlO) clusters;Decin, L.;Astron. Astrophys.,2017