\ud83d\udde3CICLO DE SEMINARIOS – SeCyT FCAG\ud83d\udde3<\/p>\n\n\n\n
\u2728Planetary Nebulae Physically Associated with Star Clusters: New Insights into Low-to-Intermediate Mass Stellar Evolution Studies.
A cargo de la Dra. Vasiliki Fragkou (Valongo Observatory, Brazil).<\/p>\n\n\n\n
\ud83d\uddd3 Mi\u00e9rcoles 15 de Abril
\u23f0 13:00 h
\ud83d\udccd Sal\u00f3n Meridiano – FCAG<\/p>\n\n\n\n
\u00a1Te esperamos!<\/p>\n\n\n\n
RESUMEN<\/strong> \ud83d\udde3CICLO DE SEMINARIOS – SeCyT FCAG\ud83d\udde3 \u2728Planetary Nebulae Physically Associated with Star Clusters: New Insights into Low-to-Intermediate Mass Stellar Evolution Studies.A cargo de la Dra. Vasiliki Fragkou (Valongo Observatory, Brazil). \ud83d\uddd3 Mi\u00e9rcoles 15 de Abril\u23f0 13:00 h\ud83d\udccd Sal\u00f3n Meridiano – FCAG \u00a1Te esperamos! RESUMENStellar evolution studies are hindered by the lack of a solid link… Read More »SEMINARIOS SECyT – Vasiliki Fragkou<\/span><\/a><\/p>\n","protected":false},"author":3,"featured_media":16935,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"neve_meta_sidebar":"","neve_meta_container":"","neve_meta_enable_content_width":"","neve_meta_content_width":0,"neve_meta_title_alignment":"","neve_meta_author_avatar":"","neve_post_elements_order":"","neve_meta_disable_header":"","neve_meta_disable_footer":"","neve_meta_disable_title":"","neve_meta_reading_time":"","_themeisle_gutenberg_block_has_review":false,"footnotes":""},"categories":[5005],"tags":[],"ubicacionentradas":[20],"class_list":["post-16934","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-ciencia_y_tecnica","ubicacionentradas-eventos"],"aioseo_notices":[],"aioseo_head":"\n\t\t\n\t\n\t\n\t\n\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t
Stellar evolution studies are hindered by the lack of a solid link connecting the initial and final stellar properties, which is crucial for understanding how stars evolve and contribute to the chemical enrichment of galaxies. This key problem can be resolved by studying stars that are both members of well-characterized star clusters and at the final stages of their evolution. In such cases, their final properties can be determined from direct measurements, while the properties of their progenitors can be inferred from independent cluster studies. Here, we focus on the study of planetary nebulae that are confirmed members of Galactic open star clusters. Although such systems are very rare, with only five confirmed to date, they reveal extreme and otherwise undetectable planetary nebula properties and provide new insights into the evolution of low-to-intermediate mass stars.<\/p>\n","protected":false},"excerpt":{"rendered":"