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BEGIN:VEVENT
UID:20260518T142116-04-16482LwJj7@https://astronomia.uc.cl/2jucext1/institu
 toastrofisica/
DTSTAMP:20260518T182116Z
DESCRIPTION:The study of Planetary Nebulae (PNe) provides vital clues for u
 nderstanding late stage stellar evolution and stellar mass loss. Despite t
 heir significance\, various issues concerning these objects remain unsolve
 d. Interstellar extinction by dust hampers the detection of many Galactic 
 PNe at optical wavelengths while their largely unknown distances and proge
 nitor masses are two key parameters that hamper deeper understanding.&nbsp
 \; Identification of dust obscured PNe can be partially solved with observ
 ations at longer wavelengths where extinction effects are less serious and
  by multi-wavelength techniques proposed for their detection. Here\, the e
 fficacy of these methods is evaluated for identification of new Galactic P
 N candidates.&nbsp\; PNe in Galactic star clusters have distances and prog
 enitor masses determined independently from cluster color-magnitude diagra
 ms. Here\, we study the first confirmed PN-open cluster pair (PHR1315-6555
  – AL 1) identifying its central star and measuring its physical propertie
 s. We also demonstrate in detail the physical association of PN BMP J1613-
 5406 with Galactic open cluster NGC 6067. The PN’s progenitor mass is ~5.6
  Msun. Finally\, we provide preliminary details on several additional case
 s of possible PN-cluster associations we have uncovered. Our new PN-open c
 luster associations contribute to the improvement of the initial-to-final 
 mass relation and our multi-wavelength study suggests that a new era begin
 s for the identification of Galactic PNe hidden by dust. https://astronomi
 a.uc.cl/2jucext1/institutoastrofisica/es/instituto/seminarios/evento/355-g
 alactic-planetary-nebulae-with-emphasis-on-those-that-are-members-of-open-
 star-clusters-vasiliki-fragkou-university-of-hong-kong
DTSTART:20190606T171500Z
DTEND:20190606T174500Z
LOCATION:Seminar Room (Instituto de Astrofísica\, Pontificia Universidad Ca
 tólica\, Vicuña Mackenna 4860\, Santiago\, Chile)
SUMMARY:Galactic Planetary Nebulae with Emphasis on those that are Members 
 of Open Star Clusters  (Vasiliki Fragkou\; University of Hong Kong)
URL:https://astronomia.uc.cl/2jucext1/institutoastrofisica/es/instituto/sem
 inarios/evento/355-galactic-planetary-nebulae-with-emphasis-on-those-that-
 are-members-of-open-star-clusters-vasiliki-fragkou-university-of-hong-kong
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