{ "id": "1109.2868", "version": "v1", "published": "2011-09-13T17:59:56.000Z", "updated": "2011-09-13T17:59:56.000Z", "title": "Unraveling the Geometry of the Crab Nebula's \"Inner Ring\"", "authors": [ "Martin C. Weisskopf", "Ronald F. Elsner", "Jeffery J. Kolodziejczak", "Stephen L. O'Dell", "Allyn F. Tennant" ], "comment": "12 pages, f figures, submitted to the Astrophysical Journal", "categories": [ "astro-ph.HE" ], "abstract": "Chandra images of the Crab Nebula resolve the detailed structure of its \"inner ring\", possibly a termination shock where pulsar-accelerated relativistic particles begin to emit X radiation. Analysis of these images finds that the center of the ellipse-presumably a circular ring in projection-lies about 0.9\" (10 light-days at 2 kpc) from the pulsar's image, at a position angle of about 300{\\deg} (East of North). This analysis also measures properties of the ellipse: The position angle of the semi-major axis is about 210{\\deg} (East of North); the aspect ratio, 0.49. In a simple-albeit, not unique-de-projection of the observed geometry, a circular ring is centered on the axis of symmetry of the pulsar wind nebula. This ring is not equatorial but rather lies near +4.5{\\deg} latitude in pulsar-centered coordinates. Alternative geometries are briefly discussed.", "revisions": [ { "version": "v1", "updated": "2011-09-13T17:59:56.000Z" } ], "analyses": { "keywords": [ "inner ring", "position angle", "pulsar wind nebula", "pulsar-accelerated relativistic particles begin", "crab nebula resolve" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/746/1/41", "journal": "The Astrophysical Journal", "year": 2012, "month": "Feb", "volume": 746, "number": 1, "pages": 41 }, "note": { "typesetting": "TeX", "pages": 12, "language": "en", "license": "arXiv", "status": "editable", "inspire": 927209, "adsabs": "2012ApJ...746...41W" } } }