{ "id": "2004.13707", "version": "v1", "published": "2020-04-28T17:59:42.000Z", "updated": "2020-04-28T17:59:42.000Z", "title": "Three-dimensional analysis of the Minispiral at the Galactic Center: orbital parameters, periods and the mass of the black hole", "authors": [ "Maria Selina Nitschai", "Nadine Neumayer", "Anja Feldmeier-Krause" ], "comment": "14 pages, 12 figures, 2 tables. Accepted for publication in ApJ", "categories": [ "astro-ph.GA" ], "abstract": "In this paper we simultaneously fit the orbits and line-of-sight velocities of the ionized gas around the supermassive black hole, Sagittarius A$^{\\ast}$ (Sgr A$^{\\ast}$), at the center of the Milky Way. The data we use are taken with the K-band Multi Object Spectrograph (KMOS), presented in Feldmeier-Krause et al. (2015) and cover the central $\\sim$ 2 pc of the Milky Way. From the brightest gas emission line in the K-band, the Br$\\gamma$ line, we derive the spatial distribution and line-of-sight velocities of the gas in the minispiral. Using the flux distribution and the line-of-sight velocity information, we perform a fit to the three main gas streamers in the minispiral, the Northern Arm, Eastern Arm, and Western Arc, using a Bayesian modelling method, and are able to reconstruct the three-dimensional orbits of these gas streamers. With the best fit orbital parameters and the measured line-of-sight velocities, we constrain the mass of Sgr A$^{\\ast}$. The orbit of the Eastern Arm is the one that is best constrained using our data. It gives a best-fit orbital period of $17.4_{-11.6}^{+31.0}\\cdot 10^3$ years and results in an enclosed mass of $14.9_{-10.4}^{+69.4}\\cdot 10^6 M_{\\odot}.$", "revisions": [ { "version": "v1", "updated": "2020-04-28T17:59:42.000Z" } ], "analyses": { "keywords": [ "black hole", "three-dimensional analysis", "galactic center", "line-of-sight velocity", "minispiral" ], "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable" } } }