The split red clump of the Galactic bulge from OGLE-III
The red clump (RC) is found to be split into two components along several sightlines toward the Galactic bulge. This split is detected with high significance toward the areas (-3.5 < l < 1, b < -5) and (l, b) = (0, +5.2), i.e., along the bulge minor axis
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal Letters|
|01_Nataf_The_split_red_clump_of_the_2010.pdf||3.54 MB||Adobe PDF||Request a copy|
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