{ "id": "2003.10311", "version": "v1", "published": "2020-03-23T14:57:21.000Z", "updated": "2020-03-23T14:57:21.000Z", "title": "Galactic Center IRS13E: Colliding Stellar Winds or an Intermediate Mass Black Hole?", "authors": [ "Zhenlin Zhu", "Zhiyuan Li", "Anna Ciurlo", "Mark R. Morris", "Mengfei Zhang", "Tuan Do", "Andrea M. Ghez" ], "comment": "23 pages, 9 figures, Submitted to ApJ", "categories": [ "astro-ph.HE", "astro-ph.GA" ], "abstract": "A small cluster of massive stars residing in the Galactic center, collectively known as IRS13E, is of special interest due to its close proximity to Sgr A* and the possibility that an embedded intermediate-mass black hole (IMBH) binds its member stars. It has been suggested that colliding winds from two member stars, both classified as Wolf-Rayet type, are responsible for the observed X-ray, infrared and radio emission from IRS13E. We have conducted an in-depth study of the X-ray spatial, temporal and spectral properties of IRS13E, based on 5.6 Ms of ultra-deep Chandra observations obtained over 20 years. These X-ray observations show no significant evidence for source variability. We have also explored the kinematics of the cluster members, using Keck near-infrared imaging and spectroscopic data on a 14-yr baseline that considerably improve the accuracy of stars' proper motions. The observations are interpreted using 3-dimensional hydrodynamical simulations of colliding winds tailored to match the physical conditions of IRS13E, leading us to conclude that the observed X-ray spectrum and morphology can be well explained by the colliding wind scenario, in the meantime offering no support for the presence of a putative IMBH. An IMBH more massive than a few $10^3{\\rm~M_\\odot}$ is also strongly disfavored by the stellar kinematics.", "revisions": [ { "version": "v1", "updated": "2020-03-23T14:57:21.000Z" } ], "analyses": { "keywords": [ "intermediate mass black hole", "galactic center irs13e", "colliding stellar winds", "colliding wind", "member stars" ], "note": { "typesetting": "TeX", "pages": 23, "language": "en", "license": "arXiv", "status": "editable" } } }