{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,10,9]],"date-time":"2026-10-09T19:17:19Z","timestamp":1791573439436,"version":"4.3.4"},"reference-count":78,"publisher":"American Association for the Advancement of Science (AAAS)","issue":"6620","content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Science"],"published-print":{"date-parts":[[2022,11,11]]},"abstract":"<jats:p>A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays. We report a polarimetric observation of the XRB Cygnus X-1 using the Imaging X-ray Polarimetry Explorer. The electric field position angle aligns with the outflowing jet, indicating that the jet is launched from the inner x-ray\u2013emitting region. The polarization degree is 4.01 \u00b1 0.20% at 2 to 8 kiloelectronvolts, implying that the accretion disk is viewed closer to edge-on than the binary orbit. These observations reveal that hot x-ray\u2013emitting plasma is spatially extended in a plane perpendicular to, not parallel to, the jet axis.<\/jats:p>","DOI":"10.1126\/science.add5399","type":"journal-article","created":{"date-parts":[[2022,11,3]],"date-time":"2022-11-03T18:00:25Z","timestamp":1667498425000},"page":"650-654","source":"Crossref","is-referenced-by-count":179,"title":["Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1"],"prefix":"10.1126","volume":"378","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-1084-6507","authenticated-orcid":true,"given":"Henric","family":"Krawczynski","sequence":"first","affiliation":[{"name":"Department of Physics and McDonnell Center for the Space Sciences, Washington University in St. Louis, St. Louis, MO 63130, 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