Infrared spectroscopy of asymptotic giant branch stars in the Galactic bulge
We have selected a homogeneous sample of asymptotic giant branch (AGB) stars in theGalactic bulge population from the ISOGAL survey. Our target stars cover a wide range of mass-loss rates (~10-8-10-4 M⊙ yr-1) and differ primarily by their age on the AGB
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Golriz_Infrared_spectroscopy_of_2014.pdf||7.59 MB||Adobe PDF||Request a copy|
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