{ "id": "1002.0551", "version": "v3", "published": "2010-02-02T20:55:55.000Z", "updated": "2010-05-24T07:26:33.000Z", "title": "Probing the Galaxy's bars via the Hercules stream", "authors": [ "Esko Gardner", "Chris Flynn" ], "comment": "9 pages, 10 figures, Accepted to MNRAS, Corrected for errata", "doi": "10.1111/j.1365-2966.2010.16470.x", "categories": [ "astro-ph.GA" ], "abstract": "It has been suggested that a resonance between a rotating bar and stars in the solar neighbourhood can produce the so called 'Hercules stream'. Recently, a second bar may have been identified in the Galactic centre, the so called 'long bar', which is longer and much flatter than the traditional Galactic bar, and has a similar mass. We looked at the dynamical effects of both bars, separately and together, on orbits of stars integrated backwards from local position and velocities, and a model of the Galactic potential which includes the bars directly. Both bars can produce Hercules like features, and allow us to measure the rotation rate of the bar(s). We measure a pattern speed, for both bars, of 1.87 +/- 0.02 times the local circular frequency. This is on par with previous measurements for the Galactic bar, although we do adopt a slightly different Solar motion. Finally, we identify a new kinematic feature in local velocity space, caused by the long bar, which is tempting to identify with the high velocity 'Arcturus' stream.", "revisions": [ { "version": "v3", "updated": "2010-05-24T07:26:33.000Z" } ], "analyses": { "keywords": [ "hercules stream", "galaxys bars", "long bar", "high velocity arcturus", "local velocity space" ], "tags": [ "journal article" ], "publication": { "publisher": "Wiley-Blackwell", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2010, "month": "Jun", "volume": 405, "number": 1, "pages": 545 }, "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable", "inspire": 844462, "adsabs": "2010MNRAS.405..545G" } } }