Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1

We present new high angular resolution and high sensitivity radio observations toward the neutron star RX J0007.0+7303, carried out with the Karl G. Jansky Very Large Array at 1.5 GHz. This source powers a pulsar wind nebula (PWN) only detected in the X-ray and gamma-ray domains. The new high qualit...

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Detalles Bibliográficos
Autores principales:	Giacani, E., Rovero, A.C., Cillis, A., Pichel, A., Dubner, G.
Formato:	CONF
Materias:	CTA 1 Pulsar wind nebula Radio observations Cosmic rays Cosmology Pulsars Radio Signal to noise ratio High sensitivity Neutron stars Noise levels Pulsar wind nebulae Radio observation Very large arrays Gamma rays
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_97885890_v2013-October_n_p_Giacani
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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