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SPECTRA OF THE HB 21 SUPERNOVA REMNANT: EVIDENCE OF SPECTRUM FLATTENING AT THE LOW FREQUENCIES

We use observations of the continuum radio emission at 1420, 820, 408, 34.5 and 22 MHz to estimate the mean brightness temperatures of the HB 21 supernovaremnant (SNR) at five frequencies. We also present mean spectral index of HB 21. The spectra of HB 21 are estimated from mean temperatures versus...

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Bibliografske podrobnosti
izdano v:Revista Mexicana de Astronomía y Astrofísica
Principais autores: D. Borka, V. Borka Jovanovic, D. Urosevic
Format: Artigo
Jezik:Inglês
Izdano: Universidad Nacional Autónoma de México 2012
Teme:
Online dostop:https://www.redalyc.org/articulo.oa?id=57124416005
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