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Dimitrios Giannios

10 ta ish

Purdue University West Lafayette

AkademScholarda batafsil koʻrsatkichlar

  1. Relativistic jets shine through shocks or magnetic reconnection?

    Lorenzo Sironi, Μαρία Πετροπούλου, Dimitrios Giannios

    MaqolaOchiq kirish20155 iqtibos
    ABI

  2. Blazar flares powered by plasmoids in relativistic reconnection

    Μαρία Πετροπούλου, Dimitrios Giannios, Lorenzo Sironi

    MaqolaOchiq kirish20163 iqtibos
    ABI

  3. Radiation and Polarization Signatures from Magnetic Reconnection in Relativistic Jets. II. Connection with γ-Rays

    H. C. Zhang, Xiaocan Li, Dimitrios Giannios +5

    MaqolaOchiq kirish20223 iqtibos
    ABI

  4. A STRONG OPTICAL FLARE BEFORE THE RISING AFTERGLOW OF GRB 080129

    J. Greiner, T. Krühler, S. McBreen +11

    MaqolaOchiq kirish20092 iqtibos
    ABI

  5. Kink instabilities in relativistic jets can drive quasi-periodic radiation signatures

    Lingyi Dong, H. C. Zhang, Dimitrios Giannios

    MaqolaOchiq kirish20202 iqtibos
    ABI

  6. The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin

    Wen‐fai Fong, P. K. Blanchard, K. D. Alexander +25

    MaqolaOchiq kirish20192 iqtibos
    ABI

  7. Plasmoid statistics in relativistic magnetic reconnection

    Μαρία Πετροπούλου, Ian Christie, Lorenzo Sironi +1

    MaqolaOchiq kirish20182 iqtibos
    ABI

  8. Large-amplitude Blazar Polarization Angle Swing as a Signature of Magnetic Reconnection

    H. C. Zhang, Xiaocan Li, Fan Guo +1

    MaqolaOchiq kirish20182 iqtibos
    ABI

  9. Radiation and Polarization Signatures from Magnetic Reconnection in Relativistic Jets. I. A Systematic Study

    H. C. Zhang, Xiaocan Li, Dimitrios Giannios +3

    MaqolaOchiq kirish20202 iqtibos
    ABI

  10. Thermal electrons in an ultra-relativistic shock shape the optical afterglow of GRB 250702F

    Martin Jelínek, Annarita Ierardi, Filip Novotný +8

    MaqolaOchiq kirishGamma-ray bursts and supernovaeAstronomy and Astrophysics20260 iqtibos
    ABI