Asymmetrical Post-main-sequence Nebulae 9

City: 
Granada
Date: 
22/09/2025 to 26/09/2025
Web site: 
https://www.granadacongresos.com/apn9
SOC: 
Martin A Guerrero (chair) Instituto de Astrofísica de Andalucía (IAA - CSIC, Granada, Spain) Noam Soker (co-chair) Technion, Israel Institute of Technology (Haifa, Israel) Orsola de Marco Macquarie University (Sydney, NSW, Australia) Denise R. Gonçalves Universidade Federal do Rio de Janeiro (Rio de Janeiro, Brazil) David Jones Instituto de Astrofísica de Canarias (IAC, Tenerife, Spain) Joel H. Kastner Rochester Institute of Technology (Rochester, NY, USA) Jason Nordhaus Rochester Institute of Technology (Rochester, NY, USA) Quentin Parker The University of Hong Kong (Hong Kong) Nicole Reindl Zentrum für Astronomie, Ruprecht-Karls-Universität (Heidelberg, Germany) Carmen Sánchez Contreras Centro de Astrobiología (CAB-CSIC-INTA, Spain) Albert Zijlstra The University of Manchester (Manchester, UK)
LOC: 
Faezeh Bidjarchian Instituto de Astrofísica de Andalucía (IAA - CSIC, Granada, Spain) Janis B Rodríguez González Instituto de Astrofísica de Andalucía (IAA - CSIC, Granada, Spain) Edgar I Santamaria Instituto de Radioastronomía y Astrofísica (IRyA - UNAM, Mexico)
A meeting devoted to the shaping effects of stellar outflows from evolved stars in the formation of asymmetrical post-main-sequence nebulae including planetary nebulae, nebulae around massive stars, nova remnants, symbiotic stars, ... 1.- Puzzling evolved star nebulae that challenge our present knowledge: morphology, kinematics, chemistry, time-scales, exotic central stars, ... statistics: common and uncommon 2.- PNe related/unrelated objects: novae, SNR, LRN (mergers), massive stars, symbiotics, ... transient nebulae and other eruptive objects 3.- Shaping Agents: mass-loss mechanisms role of binarity -- binary mass-transfer, common envelope magnetic fields -- strength, structure other agents disks, circumbinary disks, jet launching 4.- Nebular sequences: connecting the shape of sources in the AGB, post AGB, proto PN and PN phases evolutionary time-scales 5.- Binarity: observational and theoretical expectations links to common envelope, time-scales, mergers, exotic central stars 6.- Future: maximazing science from available and planned facilities