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Black hole spin-orbit misalignment in the x-ray binary MAXI J1820+070
The observational signatures of black holes in x-ray binary systems depend on their masses, spins, accretion rate, and the misalignment angle between the black hole spin and the orbital angular momentum. We present optical polarimetric observations of the black hole x-ray binary MAXI J1820+070, from...
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Published in: | Science (American Association for the Advancement of Science) 2022-02, Vol.375 (6583), p.874-876 |
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creator | Poutanen, Juri Veledina, Alexandra Berdyugin, Andrei V Berdyugina, Svetlana V Jermak, Helen Jonker, Peter G Kajava, Jari J E Kosenkov, Ilia A Kravtsov, Vadim Piirola, Vilppu Shrestha, Manisha Perez Torres, Manuel A P Tsygankov, Sergey S |
description | The observational signatures of black holes in x-ray binary systems depend on their masses, spins, accretion rate, and the misalignment angle between the black hole spin and the orbital angular momentum. We present optical polarimetric observations of the black hole x-ray binary MAXI J1820+070, from which we constrain the position angle of the binary orbital. Combining this with previous determinations of the relativistic jet orientation, which traces the black hole spin, and the inclination of the orbit, we determine a lower limit of 40° on the spin-orbit misalignment angle. The misalignment must originate from either the binary evolution or black hole formation stages. If other x-ray binaries have similarly large misalignments, these would bias measurements of black hole masses and spins from x-ray observations. |
doi_str_mv | 10.1126/science.abl4679 |
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We present optical polarimetric observations of the black hole x-ray binary MAXI J1820+070, from which we constrain the position angle of the binary orbital. Combining this with previous determinations of the relativistic jet orientation, which traces the black hole spin, and the inclination of the orbit, we determine a lower limit of 40° on the spin-orbit misalignment angle. The misalignment must originate from either the binary evolution or black hole formation stages. If other x-ray binaries have similarly large misalignments, these would bias measurements of black hole masses and spins from x-ray observations.</description><identifier>ISSN: 0036-8075</identifier><identifier>ISSN: 1095-9203</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.abl4679</identifier><identifier>PMID: 35201859</identifier><language>eng</language><publisher>United States: The American Association for the Advancement of Science</publisher><subject>Accretion disks ; Binary stars ; Black holes ; Companion stars ; Misalignment ; X ray binaries ; X ray stars ; X-ray astronomy ; X-rays</subject><ispartof>Science (American Association for the Advancement of Science), 2022-02, Vol.375 (6583), p.874-876</ispartof><rights>Copyright © 2022 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. 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We present optical polarimetric observations of the black hole x-ray binary MAXI J1820+070, from which we constrain the position angle of the binary orbital. Combining this with previous determinations of the relativistic jet orientation, which traces the black hole spin, and the inclination of the orbit, we determine a lower limit of 40° on the spin-orbit misalignment angle. The misalignment must originate from either the binary evolution or black hole formation stages. If other x-ray binaries have similarly large misalignments, these would bias measurements of black hole masses and spins from x-ray observations.</description><subject>Accretion disks</subject><subject>Binary stars</subject><subject>Black holes</subject><subject>Companion stars</subject><subject>Misalignment</subject><subject>X ray binaries</subject><subject>X ray stars</subject><subject>X-ray 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subjects | Accretion disks Binary stars Black holes Companion stars Misalignment X ray binaries X ray stars X-ray astronomy X-rays |
title | Black hole spin-orbit misalignment in the x-ray binary MAXI J1820+070 |
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