Artículo

Radio Observations of a galactic high energy gamma-ray source

Giacani, Elsa BeatrizIcon ; Rovero, Adrian CarlosIcon
Fecha de publicación: 12/2001
Editorial: Societa Italiana di Fisica
Revista: Il Nuovo Cimento
ISSN: 2037-4909
Idioma: Inglés
Tipo de recurso: Artículo publicado
Clasificación temática:

Resumen

PSR B1706-44 is one of the very few galactic pulsars that has been discovered at TeV energies. PSR B1706-44 has been also detected in the Xray domain. It has been suggested that the high energy radiation could be due to inverse Compton radiation from a pulsar wind nebula (PWN).We report on VLA high-resolution observations of a region around the pulsar PSR B1706-44 at 1.4, 4.8 and 8.4 GHz. The pulsar appears embedded in a synchrotron nebula. We propose that this synchrotron nebula is the radio counterpart of the high energy emission powered by the spin-down energy of the pulsar.
Palabras clave: Radio Sources
 
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Licencia
info:eu-repo/semantics/openAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)
Identificadores
URI: http://hdl.handle.net/11336/22376
URL: https://en.sif.it/journals/ncc/econtents/2001/024/04-05/article/18
Colecciones
Articulos(IAFE)
Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)
Citación
Giacani, Elsa Beatriz; Rovero, Adrian Carlos; Radio Observations of a galactic high energy gamma-ray source; Societa Italiana di Fisica; Il Nuovo Cimento; 24; 4-5; 12-2001; 657-659
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