Abstract
We present results of a study of obscured Asymptotic Giant Branch (AGB) stars in the Large and Small Magellanic Clouds (LMC and SMC). In contrast with optically bright AGB stars (e.g. Blanco et al. 1980; Costa & Frogel 1996 and references therein) our sample of IRAS detected stars (Reid 1991; Wood et al. 1992; Loup et al. 1997; Zijlstra et al. 1996; van Loon et al. 1997a) represents stars that are in the very last stage of their AGB evolution. Elsewhere in this volume, Groenewegen reviews the magellanic AGB stars, and Trams et al. present first ISO results. Here we present results obtained from ground based observations.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
