{ "id": "1110.4313", "version": "v1", "published": "2011-10-19T15:43:35.000Z", "updated": "2011-10-19T15:43:35.000Z", "title": "Trigonometric Parallaxes of Massive Star-Forming Regions. IX. The Outer Arm in the First Quadrant", "authors": [ "A. Sanna", "M. J. Reid", "T. M. Dame", "K. M. Menten", "A. Brunthaler", "L. Moscadelli", "X. W. Zheng", "Y. Xu" ], "comment": "19 pages, 5 figures, 4 tables, accepted by The Astrophysical Journal", "categories": [ "astro-ph.GA" ], "abstract": "We report a trigonometric parallax measurement with the Very Long Baseline Array for the water maser in the distant high-mass star-forming region G75.30+1.32. This source has a heliocentric distance of 9.25+-0.45 kpc, which places it in the Outer arm in the first Galactic quadrant. It lies 200 pc above the Galactic plane and is associated with a substantial HI enhancement at the border of a large molecular cloud. At a Galactocentric radius of 10.7 kpc, G75.30+1.32 is in a region of the Galaxy where the disk is significantly warped toward the North Galactic Pole. While the star-forming region has an instantaneous Galactic orbit that is nearly circular, it displays a significant motion of 18 km/s toward the Galactic plane. The present results, when combined with two previous maser studies in the Outer arm, yield a pitch angle of about 12 degrees for a large section of the arm extending from the first quadrant to the third.", "revisions": [ { "version": "v1", "updated": "2011-10-19T15:43:35.000Z" } ], "analyses": { "keywords": [ "outer arm", "first quadrant", "massive star-forming regions", "trigonometric parallaxes", "galactic plane" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/745/1/82", "journal": "The Astrophysical Journal", "year": 2012, "month": "Jan", "volume": 745, "number": 1, "pages": 82 }, "note": { "typesetting": "TeX", "pages": 19, "language": "en", "license": "arXiv", "status": "editable", "inspire": 940548, "adsabs": "2012ApJ...745...82S" } } }