Vela Z-so young and so exotic

Details Vela Z-so young and so exotic Vela Z-so young and so exotic

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..267f&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 267-270 (2001).

Astronomy and Astrophysics

Astrophysics

3

Supernova Remnants, Supernovae, Magnetohydrodynamics And Plasmas

Scientific paper

We present a multi-frequency study of the recently discovered supernova remnant (SNR) RX J0852.0-4622 (Vela Z) superimposed on the well-known Vela SNR. The structure of SNR RX J0852.0-4622 is shell-like (barrel-shaped/bilateral) with correlation between radio-continuum, EUV and ROSAT PSPC X-ray emission. The radio-continuum coinciding with X-ray confirms that synchrotron radiation is responsible for the north and south brightened X-ray limbs. The area of RX J0852.0-4622 has filaments of optical line emission in [O III] and [S II], but some of these may be associated with the surrounding Vela SNR. .

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