{ "id": "1511.07641", "version": "v1", "published": "2015-11-24T10:47:29.000Z", "updated": "2015-11-24T10:47:29.000Z", "title": "A recent change in the optical and γ-ray polarization of the Crab nebula and pulsar", "authors": [ "Paul Moran", "Gillian Kyne", "Christian Gouiffes", "3", "Philipe Laurent", "Gregg Hallinan", "Michael Redfern", "Andrew Shearer" ], "comment": "9 pages accepted for publication in MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "We report on observations of the polarization of optical and {\\gamma}-ray photons from the Crab nebula and pulsar system using the Galway Astronomical Stokes Polarimeter (GASP), the Hubble Space Telescope/Advanced Camera for Surveys (HST/ACS) and the International Gamma-Ray Astrophysics Laboratory satellite (Integral). These, when combined with other optical polarization observations, suggest that the polarized optical emission and {\\gamma}-ray polarization changes in a similar manner. A change in the optical polarization angle has been observed by this work, from 109.5 \\pm 0.7\\deg in 2005 to 85.3 \\pm 1.4 \\deg in 2012. On the other hand, the {\\gamma}-ray polarization angle changed from 115 \\pm 11 \\deg in 2003-2007 to 80 \\pm 12 \\deg in 2012-2014. Strong flaring activities have been detected in the Crab nebula over the past few years by the high energy {\\gamma}-ray missions Agile and Fermi, and magnetic reconnection processes have been suggested to explain these observations. The change in the polarized optical and {\\gamma}-ray emission of the Crab nebula/pulsar as observed, for the first time, by GASP and Integral may indicate that reconnection is possibly at work in the Crab nebula. We also report, for the first time, a non-zero measure of the optical circular polarization from the Crab pulsar+knot system.", "revisions": [ { "version": "v1", "updated": "2015-11-24T10:47:29.000Z" } ], "analyses": { "keywords": [ "crab nebula", "international gamma-ray astrophysics laboratory satellite", "first time", "galway astronomical stokes polarimeter", "observations" ], "publication": { "doi": "10.1093/mnras/stv2780" }, "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1406099 } } }