A new determination of the distance to Kepler's supernova remnant

Using the Very Large Array, H I observations of Kepler's supernova remnant (SN 1604, 3C 358) have been carried out with an angular resolution of approximately 15″ and a velocity resolution of 1.3 km s-1. The distance to this historical supernova remnant (SNR; diameter ∼3′) has been controversia...

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Detalles Bibliográficos
Autores principales:	Reynoso, E.M., Goss, W.M.
Formato:	JOUR
Materias:	Ism: clouds ISM: H I Ism: individual 3C 358 = Kepler's supernova Supernova remnants Supernovae: individual (SN 1604)
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046256_v118_n2_p926_Reynoso
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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