Magellanic Cloud stars with TiO bands in emission: Binary post-RGB/AGB stars or young stellar objects?
14 stars from a sample of Magellanic Cloud objects selected to have a mid-infrared flux excess have been found to also show TiO bands in emission. The mid-infrared dust emission and the TiO band emission indicate that these stars have large amounts of hot
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|Access Rights:||Open Access|
|01_Wood_Magellanic_Cloud_stars_with_2013.pdf||2.15 MB||Adobe PDF|
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