Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1780478 | New Astronomy Reviews | 2006 | 5 Pages |
Abstract
There are several shrapnels around the Vela SNR that originated from the inner layer of the progenitor star. We present here the analysis of the X-ray spectrum of the Vela shrapnel A with XMM-Newton satellite. The Vela shrapnel A is one of several protrusions identified as bullets from Vela supernova explosion. We confirmed that there was a prominent Si Kα emission line showing a Si-rich plasma. The mass ratio between O and Si is 1.4:1. The shrapnel D also shows metal rich abundance. The mass ratio of O, Ne and Mg is about 7:3:1. These mass ratios can be found in the 13Mâ star. We estimate that the birth place of the shrapnel A is the mass radius of 1.5Mâ while that of the shrapnel D is the mass radius of 1.64Mâ.
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Authors
Hiroshi Tsunemi, Satoru Katsuda,