{ "id": "2410.08277", "version": "v1", "published": "2024-10-10T18:00:03.000Z", "updated": "2024-10-10T18:00:03.000Z", "title": "The Impact of Classical Bulges on Stellar Bars and Box-Peanut-X-Features in Disk Galaxies", "authors": [ "Rachel Lee McClure", "Angus Beane", "Elena D'Onghia", "Carrie Filion", "Kathryne J. Daniel" ], "comment": "13 pages, 9 figures, Submitted to MNRAS, Comments welcome!", "categories": [ "astro-ph.GA" ], "abstract": "Galactic bars and their associated resonances play a significant role in shaping galaxy evolution. Resulting resonance-driven structures, like the vertically extended Boxy/Peanut X-Feature (BPX), then serve as a useful probe of the host galaxy's history. In this study, we quantify the impact of a classical bulge on the evolution of the bar and the growth of bar resonance structures. This is accomplished with a suite of isolated N-body disk galaxy simulations with bulge mass fractions ranging from 0% to 16% of the disk mass. We apply frequency analysis to the stellar orbits to analyze the variations in resonance structure evolution. Our findings indicate that a more massive initial bulge leads to the formation of a stronger and more extended bar and that each bar drives the formation of a prominent associated BPX through resonance passage. In this work, we present evidence that the formation of a BPX is driven by planar, bar-supporting orbits evolving through interaction with horizontal and vertical bar-resonances. More orbits become vertically extended when these resonances overlap, and the rate of the orbits passing through resonance is moderated by the overall fraction of vertically extended orbits. A significant bulge stabilizes the fraction of vertically extended orbits, preventing sudden resonance-induced changes. Crucially, neither sudden resonance overlap nor prolonged resonance trapping is required for BPX formation.", "revisions": [ { "version": "v1", "updated": "2024-10-10T18:00:03.000Z" } ], "analyses": { "keywords": [ "classical bulge", "stellar bars", "resonance structure", "vertically extended orbits", "box-peanut-x-features" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }