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  1. Article ; Online: Electromagnetic counterparts of gravitational wave sources at the Very Large Telescope.

    Levan, Andrew J / Jonker, Peter G

    Nature reviews. Physics

    2020  Volume 2, Issue 9, Page(s) 455–457

    Abstract: Andrew J. Levan and Peter G. Jonker discuss, on behalf of the Electromagnetic counterparts of gravitational wave sources at the Very Large Telescope (ENGRAVE), how the collaboration was formed and what its goals are in the era of multi-messenger ... ...

    Abstract Andrew J. Levan and Peter G. Jonker discuss, on behalf of the Electromagnetic counterparts of gravitational wave sources at the Very Large Telescope (ENGRAVE), how the collaboration was formed and what its goals are in the era of multi-messenger astronomy.
    Language English
    Publishing date 2020-07-16
    Publishing country England
    Document type Journal Article
    ISSN 2522-5820
    ISSN (online) 2522-5820
    DOI 10.1038/s42254-020-0216-2
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  2. Article ; Online: Electromagnetic counterparts of gravitational wave sources at the Very Large Telescope

    Levan, Andrew J. / Jonker, Peter G.

    Nat Rev Phys

    Abstract: Andrew J. Levan and Peter G. Jonker discuss, on behalf of the Electromagnetic counterparts of gravitational wave sources at the Very Large Telescope (ENGRAVE), how the collaboration was formed and what its goals are in the era of multi-messenger ... ...

    Abstract Andrew J. Levan and Peter G. Jonker discuss, on behalf of the Electromagnetic counterparts of gravitational wave sources at the Very Large Telescope (ENGRAVE), how the collaboration was formed and what its goals are in the era of multi-messenger astronomy.
    Keywords covid19
    Publisher PMC
    Document type Article ; Online
    DOI 10.1038/s42254-020-0216-2
    Database COVID19

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  3. Article ; Online: Black hole spin-orbit misalignment in the x-ray binary MAXI J1820+070.

    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

    Science (New York, N.Y.)

    2022  Volume 375, Issue 6583, Page(s) 874–876

    Abstract: 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 ... ...

    Abstract 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.
    Language English
    Publishing date 2022-02-24
    Publishing country United States
    Document type Journal Article ; Research Support, Non-U.S. Gov't
    ZDB-ID 128410-1
    ISSN 1095-9203 ; 0036-8075
    ISSN (online) 1095-9203
    ISSN 0036-8075
    DOI 10.1126/science.abl4679
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  4. Article ; Online: A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni.

    Miller-Jones, James C A / Tetarenko, Alexandra J / Sivakoff, Gregory R / Middleton, Matthew J / Altamirano, Diego / Anderson, Gemma E / Belloni, Tomaso M / Fender, Rob P / Jonker, Peter G / Körding, Elmar G / Krimm, Hans A / Maitra, Dipankar / Markoff, Sera / Migliari, Simone / Mooley, Kunal P / Rupen, Michael P / Russell, David M / Russell, Thomas D / Sarazin, Craig L /
    Soria, Roberto / Tudose, Valeriu

    Nature

    2019  Volume 569, Issue 7756, Page(s) 374–377

    Abstract: Powerful relativistic jets are one of the main ways in which accreting black holes provide kinetic feedback to their surroundings. Jets launched from or redirected by the accretion flow that powers them are expected to be affected by the dynamics of the ... ...

    Abstract Powerful relativistic jets are one of the main ways in which accreting black holes provide kinetic feedback to their surroundings. Jets launched from or redirected by the accretion flow that powers them are expected to be affected by the dynamics of the flow, which for accreting stellar-mass black holes has shown evidence for precession
    Language English
    Publishing date 2019-04-29
    Publishing country England
    Document type Journal Article ; Research Support, U.S. Gov't, Non-P.H.S. ; Research Support, Non-U.S. Gov't
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/s41586-019-1152-0
    Database MEDical Literature Analysis and Retrieval System OnLINE

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    In stock of ZB MED Cologne/Königswinter

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    ab Jg. 2022: Lesesaal (EG)
    Zs.MG 9: Show issues
    Zs.MO 244: Show issues

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