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Sabina-M ă d ă lina Chi ţă , Norbert Langer, Allard-Jan van Marle Sterrenkundig Instituut Universiteit Utrecht. Evolution of the circumstellar medium around massive stars. NGC 7635 (The Bubble Nebula). stellar wind bubble H II region (photoionized) 3 pc wide.
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Sabina-Mădălina Chiţă , Norbert Langer, Allard-Jan van Marle Sterrenkundig Instituut Universiteit Utrecht Evolution of the circumstellar medium around massive stars
NGC 7635 (The Bubble Nebula) • stellar wind bubble • H II region (photoionized) • 3 pc wide
H-R diagram for 12 M⊙ star • Presupernova stage : • MS-> RSG-> BSG-> RSG • data credit :A.Heger, Los Alamos
Stellar wind mass-loss history • RSG-> BSG-> RSG • mass loss • velocity • photoionization
ZEUS -3D code • hydrodynamicalcode: credit Stone & Norman (1992) • solvesthe Euler equations on a fixed grid • photoionization: credit García-Segura (1999) • rotation: wind compressed disk model: credit Cassinelli & Bjorkman (1992)
1D simulation of MS • end of MS stage • photoionized region • hot bubble • MS shell
1D simulation of RSG • MS -> RSG • old MS shell • new MS shell(hot bubble shell) • no photo-ionization • RSG shell
2D simulation of pre-supernova • final stage: pre-supernova • RSG shell
2D simulation • RSG shell • 3 pc
Outlook • SN 1987 A • BSG progenitor of SN1987 A