a Study of Post-Agb Stars in the Light of GAIA DR3 Data
Low and intermediate-mass stars evolve through the Post Asymptotic Giant Branch (post-AGB) phase before they reach the Planetary Nebulae stage. After leaving the Main Sequence, they undergo intense episodes of mass loss when in the Giant Branch and, then, they enter the post-AGB stage which is a rather puzzling stellar evolutionary phase . Also, it
Manteiga, Minia et al.
Fecha de publicación:
8
2024