590 likes | 717 Views
I ntermediate-mass evolved star winds: an observer’s perspective. Jacco van Loon Keele University. Kalirai et al. (2008). Kalirai et al. (2009). Kalirai et al. (2008). A GB. Javadi et al. (2011) (from Marigo et al. 2008). Super - AGB. RSG. Sloan et al. (2009). Sculptor.
E N D
Intermediate-mass evolved star winds: an observer’s perspective Jacco van Loon Keele University
Kalirai et al. (2008) Kalirai et al. (2009)
AGB Javadi et al. (2011) (from Marigo et al. 2008) Super - AGB RSG
Sloan et al. (2009) Sculptor
Wood et al. (1992) mass loss
Fe 200 nm Vollmer et al. (2009)
dust formation radius van Loon et al. (2005)
maser Marshall et al. (2004)
Atacama Large (sub)Millimeter Array Australian SKA Pathfinder
CW Leo = IRC +10 216 Leão et al.
Ercole et al. (2012) M 4 2nd generation pristine gas 1st generation winds
Ercole et al. (2012) NGC 2808 2nd generation 1st generation winds pristine gas
Origlia et al. Reimers McDonald et al. (2009) dust
iron McDonald et al. (2010, 2011)
SMC LMC
2 micron M 33 Spitzer
Javadi et al. (2011) (from Marigo et al. 2008) super-AGB RSG AGB
RGB AGB super-AGB / RSG Javadi et al. (2012)
Action points • Wind kinematics (stellar parameters) • Dust-to-gas ratios (stellar parameters) • Mass-loss rates from not-very-dusty stars • Detailed case studies confronting models… • …and population studies confrontingmodels • Interaction with the ISMand/or companions • Super-AGB stars