Identifying the counterpart of HESS J1858+020

Aims: HESS J1858+020 is a weak γ-ray source that does not have any clear cataloged counterpart at any wavelengths. Recently, the source G35.6-0.4 was re-identified as a SNR. The HESS source lies towards the southern border of this remnant. The purpose of this work is to investigate the interstellar...

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Detalles Bibliográficos
Autores principales:	Paron, S., Giacani, E.
Formato:	JOUR
Materias:	Clouds - ISM Individual objects ISM ISM - ISM Supernova remnants - Gamma rays Clouds Elementary particles Signal to noise ratio Stars Clouds-ISM Supernova remnants Gamma rays
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v509_n1_p_Paron
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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