{ "id": "1403.2533", "version": "v1", "published": "2014-03-11T10:52:55.000Z", "updated": "2014-03-11T10:52:55.000Z", "title": "Proper motions for HST observations in three off-axis bulge fields", "authors": [ "Mario Soto", "Hugo Zeballos", "Konrad Kuijken", "R. Michael Rich", "Andrea Kunder", "Tri Astraatmadja" ], "comment": "14 pages, 14 figures, published in Astronomy & Astrophysics", "journal": "A&A 562, A41 (2014)", "categories": [ "astro-ph.GA" ], "abstract": "Aims. This is the second in a series of papers that attempt to unveil the kinematic structure of the Galactic bulge through studying radial velocities and proper motions. We report here ~15000 new proper motions for three low foreground-extinction off-axis fields of the Galactic bulge. Methods. Proper motions were derived from a combination of Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2) and Advanced Camera for Surveys (ACS) images taken 8 and 9 years apart, and ACS observations taken 9 and 10 years apart, and they reach accuracies better than 0.9 mas/yr for more than ~10000 objects with magnitudes F814W < 24. Results. The proper motion distributions in these fields are similar to those of Galactic minor axis bulge fields. We observe the rotation of main sequence stars below the turn-off within the Galactic bulge, as in the minor axis fields. Conclusions. Our stellar proper motions measurements show a significant bulge rotation for fields as far from the galactic plane as b=-8.", "revisions": [ { "version": "v1", "updated": "2014-03-11T10:52:55.000Z" } ], "analyses": { "keywords": [ "proper motion", "off-axis bulge fields", "wide field planetary camera", "hst observations", "minor axis bulge fields" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/201117339", "journal": "Astronomy and Astrophysics", "year": 2014, "month": "Feb", "volume": 562 }, "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014A&A...562A..41S" } } }