Document type

Article

Version

Published version

Publication date

Publication license

cc-by (c) Paredes i Poy, Josep Maria et al., 2025
Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/221067

Exploring the non-thermal physics behind the pulsar wind nebula PSR J2030+4415 through radio observations

Journal Title

Director/Tutor

Journal ISSN

Volume Title

Abstract

PSR J2030+4415 is a gamma-ray pulsar with an X-ray pulsar wind nebula elongated North-South. The system shows a prominent X-ray filament oriented at an angle of 130° to the nebula axis. To improve our understanding of the non-thermal processes occurring in the pulsar wind nebula, we attempt to determine the possible existence of a radio counterpart, study its morphology and obtain restrictive upper limits of the pulsar and filament emission at radio wavelengths. We have performed observations of the pulsar PSR J2030+4415 and its surroundings with the upgraded Giant Metrewave Radio Telescope (uGMRT) at two frequency bands, and put the results in context with findings at other wavelengths. We have obtained radio images at 736 and 1274 MHz revealing a structure trailing the pulsar, with a morphology overlapping the X-ray nebula. This radio structure is the radio counterpart of the X-ray PWN. The derived spectral index along this structure shows spatial variation. There are no hints of the pulsar and the filament at any of the explored radio frequencies but we have obtained restrictive upper limits. A physical scenario that combines the radio and the X-ray observations, and consistent with IR data, of the nebula and the filament is presented. We propose that particle acceleration occurs in the nebula tail due to the presence of a re-collimation shock, and the highest energy particles gradually escape from it through energy-dependent diffusion. We also find a lower limit in the energy of the particles escaping along the X-ray filament of $\sim$~GeV.

Citation

Citation

PAREDES I POY, Josep Maria, et al. Exploring the non-thermal physics behind the pulsar wind nebula PSR J2030+4415 through radio observations. Astronomy & Astrophysics. 2024. Vol. 693. ISSN 0004-6361. [consulta: 12 de maig de 2026]. Disponible a: https://hdl.handle.net/2445/221067

Export metadata

JSON - METS

Share record