New Hard X-Ray and Multiwavelength Study of the PeVatron Candidate Pulsar Wind Nebula G0.9+0.1 in the Galactic Center Region

We present a new X-ray study and multiwavelength spectral energy distribution (SED) modeling of the young pulsar wind nebula (PWN) powered by the energetic pulsar PSR J1747–2809, inside the composite supernova remnant (SNR) G0.9+0.1, located in the Galactic center region. The source is detected by N...

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Detalles Bibliográficos

Principais autores:	Giulia Brunelli, Kaya Mori, Jaegeun Park, Jordan Eagle, Moaz Abdelmaguid, Melania Nynka, Hongjun An, Aya Bamba, Joseph D. Gelfand, Gabriele Ponti, Samar Safi-Harb, Vito Sguera, Cristian Vignali, Jooyun Woo, Roberta Zanin
Formato:	Artigo
Idioma:	Inglês
Publicado:	IOP Publishing 2026-01-01
Series:	The Astrophysical Journal
Assuntos:	Pulsar wind nebulae High energy astrophysics X-ray sources Gamma-ray sources Spectral energy distribution
Acceso en liña:	https://doi.org/10.3847/1538-4357/ae38e0
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