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Bulge mass due to accreted stars is now followed
- Previously, the code was following only the mass that was formed via starbursts due to disk instabilities and mergers. That mass is by definition in the bulge. However, another growth channel for the bulge is the accretion of stars that were formed in the disk of the primary and/or secondary galaxy that because of the merger is transferred to the bulge. This is now being followed. - For that it was necessary to add in the components.h a property to track that growth channel, and galaxy_mergers was edited to explicitely track that growth.
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