{ "id": "1409.5447", "version": "v1", "published": "2014-09-18T20:09:03.000Z", "updated": "2014-09-18T20:09:03.000Z", "title": "Event-Horizon-Telescope Evidence for Alignment of the Black Hole in the Center of the Milky Way with the Inner Stellar Disk", "authors": [ "Dimitrios Psaltis", "Ramesh Narayan", "Vincent L. Fish", "Avery E. Broderick", "Abraham Loeb", "Sheperd S. Doeleman" ], "comment": "To appear in the Astrophysical Journal", "categories": [ "astro-ph.HE" ], "abstract": "Observations of the black hole in the center of the Milky Way with the Event Horizon Telescope at 1.3 mm have revealed a size of the emitting region that is smaller than the size of the black-hole shadow. This can be reconciled with the spectral properties of the source, if the accretion flow is seen at a relatively high inclination (50-60 degrees). Such an inclination makes the angular momentum of the flow, and perhaps of the black hole, nearly aligned with the angular momenta of the orbits of stars that lie within 3 arcsec from the black hole. We discuss the implications of such an alignment for the properties of the black hole and of its accretion flow. We argue that future Event-Horizon-Telescope observations will not only refine the inclination of Sgr A* but also measure precisely its orientation on the plane of the sky.", "revisions": [ { "version": "v1", "updated": "2014-09-18T20:09:03.000Z" } ], "analyses": { "keywords": [ "black hole", "inner stellar disk", "milky way", "event-horizon-telescope evidence", "accretion flow" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/798/1/15", "journal": "The Astrophysical Journal", "year": 2015, "month": "Jan", "volume": 798, "number": 1, "pages": 15 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1318307, "adsabs": "2015ApJ...798...15P" } } }