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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Fuente:
googleTipo de documento:
Other
Estado:
Acceso abierto
Áreas de conocimiento:
Áreas temáticas de Dewey:
- Mecánica clásica
- Astronomía y ciencias afines
- Cuerpos y fenómenos celestes específicos
Objetivos de Desarrollo Sostenible:
- ODS 9: Industria, innovación e infraestructura
- ODS 17: Alianzas para lograr los objetivos
- ODS 7: Energía asequible y no contaminante