Evidence for non - thermal bremsstrahlung from the supernova remnant MSH14- 63/ RCW 86
Jacco Vink (Columbia University)

Contents

Title page

Properties of RCW 86

Key Issues

Synchrotron emission

XMM-Newton

EPIC Mosaic

Spectra

Spectra continued

Fe K emission

Eq. widths

Is there a radio/X-ray correlation?

The radio/X-ray correlation continued

Can X-ray synchrotron emission be ruled out?

The case for X-ray bremsstrahlung

Conclusions

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Author: Jacco Vink

E-mail: jvink@astro.columbia.edu

Homepage: http://www.astro.columbia.edu/~jvink/

Meer informatie:
Adapted from a presentation at the Chandra Fellow Symposium, October 15, 2001, at the CfA, Cambridge, Ma.