HAWC Detection of a TeV Halo Candidate Surrounding a Radio-quiet Pulsar


Abstract:

Extended very-high-energy (VHE; 0.1–100 TeV) γ-ray emission has been observed around several middle-aged pulsars and referred to as “TeV halos.” Their formation mechanism remains under debate. It is also unknown whether they are ubiquitous or related to a certain subgroup of pulsars. With 2321 days of observation, the High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory detected VHE γ-ray emission at the location of the radio-quiet pulsar PSR J0359+ 5414 with> 6σ significance. By performing likelihood tests with different spectral and spatial models and comparing the TeV spectrum with multiwavelength observations of nearby sources, we show that this excess is consistent with a TeV halo associated with PSR J0359+ 5414, though future observation of HAWC and multiwavelength follow-ups are needed to confirm this nature. This new halo candidate is located in a noncrowded region in …

Año de publicación:

2023

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    Tipo de documento:

    Other

    Estado:

    Acceso abierto

    Áreas de conocimiento:

      Áreas temáticas de Dewey:

      • Mecánica clásica
      • Astronomía y ciencias afines
      • Cuerpos y fenómenos celestes específicos
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      Objetivos de Desarrollo Sostenible:

      • ODS 9: Industria, innovación e infraestructura
      • ODS 17: Alianzas para lograr los objetivos
      • ODS 7: Energía asequible y no contaminante
      Procesado con IAProcesado con IA