AbstractWe present multi frequency radio-continuum observations of Galactic SNR Vela Z (G266.2-1.2), associated with the prominent X-ray source RX J0852.0-4622 discovered in 1998. Our study of this Galactic supernova remnant (SNR) is based on low-resolution mosaic observations with the ATCA radio interferometer at 1384 and 2496 MHz, Parkes 4850 MHz and MOST 843 MHz survey data. We determine the radio spectral index for the most prominent features of this SNR and compare these features with X-ray observations. We note a sudden spectral turnover at higher then expected frequencies of ∼1384 MHz.
Radio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2)
Advances in Space Research ; 35 , 6 ; 1047-1051
2005-02-21
5 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Radio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2)
Online Contents | 2005
|Radio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2)
British Library Conference Proceedings | 2005
|Is Vela Jr. a young supernova remnant?
Online Contents | 2009
|Is Vela Jr. a young supernova remnant?
Elsevier | 2009
|High-Velocity Gas in the Direction to the Vela Supernova Remnant
British Library Online Contents | 1998
|