2001/03/05 by Letizia Stanghellini, Richard A. Shaw, Stanghellini, Letizia +3
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0103076
Invited talk. Proceedings of the conference "Ionized Gaseous Nebulae", Mexico City, November 21- 24, 2000; RMAA, in press
arxiv created 2001/03/05 · openalex publication_date 2001/03/05 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Planetary Nebulae (PNs) in the Magellanic Clouds are studied to understand\nstellar populations and evolution of low- and intermediate-mass stars in\ndifferent chemical environments. Using HST observations from our LMC and SMC PN\nmorphological survey and from the HST Data Archive, we look at the relations\nbetween PN morphology and their evolution and populations. In this paper we\nshow some of our recent results on these relations, in an historical context.\n