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Modelling of the OCS/SODART Observations of SN Remnants

A Finoguenov et al 1998 Phys. Scr. T77 139-141   doi: 10.1088/0031-8949/1998/T77/041  Help

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A Finoguenov1, K Borozdin1, T Litvinova1, F E Christensen2, N J Westergaard2, H Wiebicke3 and I Halm3
1 Space Research Institute, 84/32 Profsoyuznaya, 117810 Moscow, Russia
2 Danish Space Research Institute, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark
3 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany

Abstract. We study the effects of the Point Spread Function (PSF) on the performance of the Objective Crystal Spectrometer (OCS) of the SODART telescope. The advantage of OCS/SODART over XMM and AXAF instruments in studying of the diffuse sources is illustrated by modelling of the OCS/SODART observation of Tycho and Cas A Supernova Remnants (SNR).

PACS number: 95.85.Nv

Received 1 October 1997

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