Three Ph.D. positions at ROB, KUL and ULB In the late stages of their evolution, low- to intermediate-mass stars (LIMS) are in a rapid transition from the Asymptotic Giant Branch (AGB) phase to the White Dwarf (WD) phase - LIMS - Document - PDFSEARCH.IO

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	Three Ph.D. positions at ROB, KUL and ULB In the late stages of their evolution, low- to intermediate-mass stars (LIMS) are in a rapid transition from the Asymptotic Giant Branch (AGB) phase to the White Dwarf (WD) phase Add to Reading List Open Document File Size: 36,83 KB Share Result on Facebook City Bruxelles / / Country Belgium / / Currency EUR / / / Facility Royal Observatory of Belgium / / IndustryTerm thermodynamical and chemical structures / chemical mechanisms / chemical evolution / chemical processes / / Organization Institut d'Astronomie / Katholieke Universiteit Leuven / Doctoral School / / Person S. Van Eck / Herschel / H. Van Winckel / Alain Jorissen / / / Position representative / / PublishedMedium the White Dwarf / / Region central Belgium / / Technology condensation / radiation / / URL http / SocialTag Physics Space Astrophysics Nuclear physics Stellar astronomy Asymptotic giant branch Protoplanetary nebula Nucleosynthesis Star Stellar evolution

Three Ph.D. positions at ROB, KUL and ULB In the late stages of their evolution, low- to intermediate-mass stars (LIMS) are in a rapid transition from the Asymptotic Giant Branch (AGB) phase to the White Dwarf (WD) phaseAdd to Reading List