HIGHLIGHTS
- What: The authors aim to explore how the presence of gas impacts the rotation of classical bulges. To achieve this, the authors compare models of galaxies with several combinations of these parameters. While the study of box/peanut bulges is not itself the main focus of the present paper, it is relevant to bear in mind that they are present in strongly barred galaxies and coexist spatially with the classical bulges. In this subsection the authors investigate the shapes of the classical bulges, which begin with spherical symmetry in the initial conditions.
- Who: Rubens E . . .
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