Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/25377
 Title: Cassiopeia A: On the origin of the hard X-ray continuum and the implication of the observed O VIII Ly-α/Ly-β distribution Authors: Bleeker, J. A. M.Van Der Heyden KKaastra, J. S.Willingale, R.Dennerl, K.Aschenbach, B.Vink, J.Vink, J. First Published: Jan-2001 Publisher: EDP Sciences for European Southern Observatory (ESO) Citation: Astronomy & Astrophysics, 2001, 365 (1) Abstract: We present the first results on the hard X-ray continuum image (up to 15 keV) of the supernova remnant Cas A measured with the EPIC cameras onboard XMM-Newton. The data indicate that the hard X-ray tail, observed previously, that extends to energies above 100 keV does not originate in localised regions, like the bright X-ray knots and filaments or the primary blast wave, but is spread over the whole remnant with a rather flat hardness ratio of the 8-10 and 10-15 keV energy bands. This result does not support an interpretation of the hard X-radiation as synchrotron emission produced in the primary shock, in which case a limb brightened shell of hard X-ray emission close to the primary shock front is expected. In fact a weak rim of emission near the primary shock front is discernable in the hardest X-ray image but it contains only a few percent of the hard X-ray emissivity. The equivalent width of the Fe-K line blend varies by more than an order of magnitude over the remnant, it is hard to explain this as Fe-emission from the reverse shock heated ejecta given the ejecta temperature and the age of the remnant. The uniquely high wavelength-dispersive RGS-spectrometer has allowed, for the first time, to extract monochromatic images in several highly ionised element species with high spectral resolution. We present here a preliminary result on the measurement of the OVIII Ly-$\alpha$ and Ly-$\beta$ brightness distribution and brightness ratios. The large observed decrease of the Ly-$\alpha$/Ly-$\beta$ ratio going from the N to the SE can be explained by small-scale $(10\hbox{$^{\prime\prime}$})$ variations in the $N_{\rm H}$ column over the remnant and the potential presence of resonance scattering of the OVIII Ly-$\alpha$ photons in the limb brightened shell. DOI Link: 10.1051/0004-6361:20000048 ISSN: 0004-6361 Links: http://hdl.handle.net/2381/25377http://www.aanda.org/articles/aa/abs/2001/01/aaxmm50/aaxmm50.html Version: Publisher Version Status: Peer-reviewed Type: Journal Article Rights: Copyright © 2001 ESO. Reproduced with permission from Astronomy & Astrophysics, © ESO. Appears in Collections: Published Articles, Dept. of Physics and Astronomy

Files in This Item:
File Description SizeFormat