Mass loss and evolution of asymptotic giant branch stars in the Magellanic Clouds

Authors	J.T. van Loon
Supervisors	T. de Jong
Cosupervisors	L.B.F.M. Waters A.A. Zijlstra
Award date	23 September 1999
Number of pages	174
Organisations	Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Document type	PhD thesis
Note	Research conducted at: Universiteit van Amsterdam & ESO, Munchen
Language	English
Downloads	Thesis Cover Titlepage Contents Chapter 1 Introduction Chapter 2 Obscured Asymptotic Giant Branch stars in the Magellanic Clouds: New IRAS counterparts Chapter 3 Obscured Asymptotic Giant Branch stars in the Magellanic Clouds: Carbon stars and OH/IR stars Chapter 4 Luminous carbon stars in the Magellanic Clouds Chapter 5 Discovery of the first extra-galactic SiO maser Chapter 6 Discovery of H2O maser emission from the red supergiant IRAS04553-6825 in the Large Magellanic Cloud Chapter 7 ISO observations of obscured Asymptotic Giant Branch stars in the Large Magellanic Cloud Chapter 8 IRAS04496-6958: A luminous carbon star with silicate dust in the Large Magellanic Cloud Chapter 9 On the metallicity dependence of AGB mass loss Chapter 10 Mass-loss rates and luminosity functions of dust-enshrouded AGB stars and red supergiants in the LMC Chapter 11 Summary and Future Appendix A TIMMI standard stars Appendix B IR colour relations Appendix C ISO photometry Appendix D ISO spectroscopy References Samenvatting Acknowledgements Cover
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