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zadetkov: 6.239
1.
  • Swings between rotation and... Swings between rotation and accretion power in a binary millisecond pulsar
    Papitto, A; Ferrigno, C; Bozzo, E ... Nature (London), 09/2013, Letnik: 501, Številka: 7468
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    It is thought that neutron stars in low-mass binary systems can accrete matter and angular momentum from the companion star and be spun-up to millisecond rotational periods. During the accretion ...
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2.
  • A propeller scenario for th... A propeller scenario for the gamma-ray emission of low-mass X-ray binaries: the case of XSS J12270−4859
    Papitto, A; Torres, D. F; Li, Jian Monthly notices of the Royal Astronomical Society, 03/2014, Letnik: 438, Številka: 3
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    XSS J12270−4859 is the only low-mass X-ray binary (LMXB) with a proposed persistent gamma-ray counterpart in the Fermi-Large Area Telescope domain, 2FGL 1227.7−4853. Here, we present the results of ...
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3.
  • Introducing the HD+B model ... Introducing the HD+B model for pulsar wind nebulae: a hybrid hydrodynamics/radiative approach
    Olmi, B; Torres, D F Monthly notices of the Royal Astronomical Society, 05/2020, Letnik: 494, Številka: 3
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    ABSTRACT Identification and characterization of a rapidly increasing number of pulsar wind nebulae is, and will continue to be, a challenge of high-energy gamma-ray astrophysics. Given that such ...
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4.
  • On the plerionic rectangula... On the plerionic rectangular supernova remnants of static progenitors
    Meyer, D M-A; Meliani, Z; Velázquez, P F ... Monthly notices of the Royal Astronomical Society, 01/2024, Letnik: 527, Številka: 3
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    ABSTRACT Pulsar wind nebulae are a possible final stage of the circumstellar evolution of massive stars, where a fast-rotating, magnetized neutron star produces a powerful wind that interacts with ...
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5.
  • Deep Search for Gamma-Ray E... Deep Search for Gamma-Ray Emission from the Accreting X-Ray Pulsar 1A 0535+262
    Hou, X.; Zhang, W.; Torres, D. F. ... The Astrophysical journal, 02/2023, Letnik: 944, Številka: 1
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    Abstract Binary systems are a well-established subclass of gamma-ray sources. The high mass X-ray binary pulsar 1A 0535+262 has been considered to be a possible gamma-ray emitter for a long time, ...
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6.
  • CONSTRAINING THE GRB-MAGNET... CONSTRAINING THE GRB-MAGNETAR MODEL BY MEANS OF THE GALACTIC PULSAR POPULATION
    Rea, N.; Gullón, M.; Pons, J. A. ... The Astrophysical journal, 11/2015, Letnik: 813, Številka: 2
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    ABSTRACT A large fraction of Gamma-ray bursts (GRBs) displays an X-ray plateau phase within <105 s from the prompt emission, proposed to be powered by the spin-down energy of a rapidly spinning newly ...
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7.
  • Characterizing the Gamma-Ra... Characterizing the Gamma-Ray Emission Properties of the Globular Cluster M5 with the Fermi-LAT
    Hou, X.; Zhang, W.; Freire, P. C. C. ... The Astrophysical journal, 04/2024, Letnik: 964, Številka: 2
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    Abstract We analyzed the globular cluster M5 (NGC 5904) using 15 yr of gamma-ray data from the Fermi Large Area Telescope (LAT). Using rotation ephemerides generated from Arecibo and FAST radio ...
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8.
  • High energy γ-ray emission ... High energy γ-ray emission from the starburst nucleus of NGC 253
    Domingo-Santamaría, E.; Torres, D. F. Astronomy and astrophysics (Berlin), 12/2005, Letnik: 444, Številka: 2
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    Both the high density medium that characterizes the central regions of starburst galaxies and its power to accelerate particles up to relativistic energies make these objects good candidates for ...
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9.
  • The X-Ray Outburst of the G... The X-Ray Outburst of the Galactic Center Magnetar over Six Years of Chandra Observations
    Rea, N.; Coti Zelati, F.; Viganò, D. ... The Astrophysical journal, 05/2020, Letnik: 894, Številka: 2
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    The magnetar SGR J1745−2900, discovered at a distance of parsecs from the Milky Way central black hole, Sagittarius A , represents the closest pulsar to a supermassive black hole ever detected. ...
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10.
  • Reverberation of pulsar win... Reverberation of pulsar wind nebulae – III. Modelling of the plasma interface empowering a long term radiative evolution
    Bandiera, R; Bucciantini, N; Olmi, B ... Monthly notices of the Royal Astronomical Society, 08/2023, Letnik: 525, Številka: 2
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    ABSTRACT The vast majority of pulsar wind nebulae (PWNe) present in the Galaxy is formed by middle-aged systems characterized by a strong interaction of the PWN itself with the supernova remnant ...
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zadetkov: 6.239

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