Feature-tailored spectroscopic analysis of the supernova remnant Puppis A in X-rays

We introduce a distinct method for performing spatially resolved spectral analysis of astronomical sources with highly structured X-ray emission. The method measures the surface brightness of neighboring pixels to adaptively size and shape each region, thus the spectra from the bright and faint fila...

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Detalles Bibliográficos
Publicado:	2016
Materias:	ISM: individual objects: Puppis A ISM: supernova remnants X-rays: ISM Magnesium Neon Spectroscopic analysis Spectrum analysis Supernovae Astronomical sources Elemental abundance Filamentary structures ISM: individual objects Spatially resolved spectroscopy X rays: ISM X-ray emitting plasmas Atmospheric optics
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v590_n_p_Luna http://hdl.handle.net/20.500.12110/paper_00046361_v590_n_p_Luna
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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