The interior of the SNR RX J0852.0-4622 (Vela Jr) at radio wavelengths

Aims. We observed the center of the supernova remnant Vela Jr in radio continuum in order to search for a counterpart to the compact central X-ray source CXOU J085201.4-461753, possibly a neutron star candidate which could be the remnant of the supernova explosion. Methods. Observations were made wi...

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Detalles Bibliográficos
Autores principales:	Reynoso, E.M., Dubner, G., Giacani, E., Johnston, S., Green, A.J.
Formato:	JOUR
Materias:	Catalogs ISM: individual objects: Vela Jr ISM: planetary nebulae: individual: Ve 2-27 ISM: supernova remnants Stars: individual: Wray 16-30 X-rays: individual: CXOU J085201.4-461753 Astrophysics Correlation theory Light sources Neutrons Radio transmission Telescopes Radio waves
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v449_n1_p243_Reynoso
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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