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  1. Article ; Online: Thermonuclear explosions on neutron stars reveal the speed of their jets.

    Russell, Thomas D / Degenaar, Nathalie / van den Eijnden, Jakob / Maccarone, Thomas / Tetarenko, Alexandra J / Sánchez-Fernández, Celia / Miller-Jones, James C A / Kuulkers, Erik / Del Santo, Melania

    Nature

    2024  Volume 627, Issue 8005, Page(s) 763–766

    Abstract: Relativistic jets are observed from accreting and cataclysmic transients throughout the Universe, and have a profound impact on their ... ...

    Abstract Relativistic jets are observed from accreting and cataclysmic transients throughout the Universe, and have a profound impact on their surroundings
    Language English
    Publishing date 2024-03-27
    Publishing country England
    Document type Journal Article
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/s41586-024-07133-5
    Database MEDical Literature Analysis and Retrieval System OnLINE

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    In stock of ZB MED Cologne/Königswinter

    Zs.A 26: Show issues Location:
    Je nach Verfügbarkeit (siehe Angabe bei Bestand)
    bis Jg. 1994: Bestellungen von Artikeln über das Online-Bestellformular
    Jg. 1995 - 2021: Lesesall (1.OG)
    ab Jg. 2022: Lesesaal (EG)
    Zs.MG 9: Show issues
    Zs.MO 244: Show issues

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  2. Article ; Online: Cygnus X-1 contains a 21-solar mass black hole-Implications for massive star winds.

    Miller-Jones, James C A / Bahramian, Arash / Orosz, Jerome A / Mandel, Ilya / Gou, Lijun / Maccarone, Thomas J / Neijssel, Coenraad J / Zhao, Xueshan / Ziółkowski, Janusz / Reid, Mark J / Uttley, Phil / Zheng, Xueying / Byun, Do-Young / Dodson, Richard / Grinberg, Victoria / Jung, Taehyun / Kim, Jeong-Sook / Marcote, Benito / Markoff, Sera /
    Rioja, María J / Rushton, Anthony P / Russell, David M / Sivakoff, Gregory R / Tetarenko, Alexandra J / Tudose, Valeriu / Wilms, Joern

    Science (New York, N.Y.)

    2021  Volume 371, Issue 6533, Page(s) 1046–1049

    Abstract: The evolution of massive stars is influenced by the mass lost to stellar winds over their lifetimes. These winds limit the masses of the stellar remnants (such as black holes) that the stars ultimately produce. We used radio astrometry to refine the ... ...

    Abstract The evolution of massive stars is influenced by the mass lost to stellar winds over their lifetimes. These winds limit the masses of the stellar remnants (such as black holes) that the stars ultimately produce. We used radio astrometry to refine the distance to the black hole x-ray binary Cygnus X-1, which we found to be [Formula: see text] kiloparsecs. When combined with archival optical data, this implies a black hole mass of 21.2 ± 2.2 solar masses, which is higher than previous measurements. The formation of such a high-mass black hole in a high-metallicity system (within the Milky Way) constrains wind mass loss from massive stars.
    Language English
    Publishing date 2021-02-18
    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.abb3363
    Database MEDical Literature Analysis and Retrieval System OnLINE

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    In stock of ZB MED Cologne/Königswinter

    Zs.A 27: Show issues Location:
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  3. 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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    Kategorien

    In stock of ZB MED Cologne/Königswinter

    Zs.A 26: Show issues Location:
    Je nach Verfügbarkeit (siehe Angabe bei Bestand)
    bis Jg. 1994: Bestellungen von Artikeln über das Online-Bestellformular
    Jg. 1995 - 2021: Lesesall (1.OG)
    ab Jg. 2022: Lesesaal (EG)
    Zs.MG 9: Show issues
    Zs.MO 244: Show issues

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