| dc.creator |
AKTEKİN ÇALIŞKAN, Ebru |
|
| dc.date |
2024-10-02T00:00:00Z |
|
| dc.date.accessioned |
2025-02-25T10:36:11Z |
|
| dc.date.available |
2025-02-25T10:36:11Z |
|
| dc.identifier |
ad3cb687-ce88-4862-ae5c-59afc5e96b34 |
|
| dc.identifier |
10.22399/ijcesen.547 |
|
| dc.identifier |
https://avesis.sdu.edu.tr/publication/details/ad3cb687-ce88-4862-ae5c-59afc5e96b34/oai |
|
| dc.identifier.uri |
http://acikerisim.sdu.edu.tr/xmlui/handle/123456789/100944 |
|
| dc.description |
In this work, we analyze the X-ray data of supernova remnant (SNR) candidate G278.0+12.4. We examine its nature and the X-ray properties such as electron temperature kTe and abundances, using Suzaku data. We found that the X-ray emission is well represented by two-component model: an absorbed thermal plasma with about 5 keV and non-thermal plasma with a photon index ~ 0.5-1. Our spectral analysis confirms that the G278.0+12.4 is likely to be an SNR. We found non-thermal X-ray emission from the spectra, which indicates that a pulsar wind nebula scenario is possible for G278.0+12.4. In order to make predictions for future missions, we perform XRISM and Athena simulations. We present our results on the nature of G278.0+12.4. |
|
| dc.language |
eng |
|
| dc.rights |
info:eu-repo/semantics/openAccess |
|
| dc.title |
X-ray Investigation of the Supernova Remnant Candidate G278.0+12.4 and Prospect of Future Missions |
|
| dc.type |
info:eu-repo/semantics/article |
|