| dc.contributor.author | BALMAN, Şölen | |
| dc.date.accessioned | 2021-03-03T07:43:14Z | |
| dc.date.available | 2021-03-03T07:43:14Z | |
| dc.identifier.citation | BALMAN Ş., "Discovery of localized non-thermal X-ray emission from the nova remnant of GK Persei (1901)", Conference on Astrophysics of Cataclysmic Variables and Related Objects, Strasbourg, Fransa, 11 - 16 Temmuz 2004, cilt.330, ss.433-434 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_137f80b2-45e9-4229-84af-5862f8c98c95 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/18555 | |
| dc.description.abstract | The X-ray nebula associated with the nova shell of GK Persei (1901) is lumpy and asymmetric with most of the emission coming from the SW. The brightest X-ray emission region that appears as all arc is co-spatial with the brightest non-therinal radio emitting region and found to be a source of non-thermal X-ray emission with a power law photon index of 2.3(-1.3)(+0-9) with L similar to 4 x 10(30) erg s(-1) at 470 pc. The unexpectedly low temperature of the forward shock (0.1-0.3 keV) is suggestive of particle acceleration occurring in this region, too. The total X-ray spectrum of the nebula consists of two prominent components of emission (other than the localized non-thermal emission). | |
| dc.language.iso | eng | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.subject | Uzay bilimi | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Fizik | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler | |
| dc.title | Discovery of localized non-thermal X-ray emission from the nova remnant of GK Persei (1901) | |
| dc.type | Bildiri | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 330 | |
| dc.contributor.firstauthorID | 2213018 | |
