The central stars

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Imaging of molecules and dustIRC+10216 inscattered interstellar lightmolecular line intensity peakson scattered lightMauron & Huggins
Comparisons of gas and dust distributionsR Scl HST/ACS imagef606wshell diameter ≈ 38”shell age ≈ 1800 yrTT Cyg PdB mapshell diameter = 68”shell age ≈ 8000 yrCO(1-0)
Page 1 and 2: ALMA and AGB starsHans OlofssonOnsa
Page 3 and 4: The importance of AGB stars- They a
Page 5 and 6: The stellar mass lossThe mass loss
Page 7 and 8: AGB stars are dynamical objectsThis
Page 9 and 10: ALMA and the central starsSize (ten
Page 11 and 12: ALMA and the CSEsM(t,θ,φ,M MS ,Z,
Page 13 and 14: ALMA and the CSEsNote thatS ∗ ∝
Page 15 and 16: ALMA and the CSEsObservational spac
Page 17 and 18: ALMA and the CSEsSizes of the emitt
Page 19 and 20: Circumstellar molecules∑ = 69 cir
Page 21 and 22: Circumstellar SiO abundance estimat
Page 23 and 24: Circumstellar isotope ratiosEven a
Page 25 and 26: ALMA and the circumstellar structur
Page 27: ALMA and the circumstellar structur
Page 31 and 32: Termination of the AGB phaseIRC+102
Page 33 and 34: Post-AGB circumstellar chemistry11

The central stars

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