Zobrazeno 1 - 10
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pro vyhledávání: '"Ergin, Tulun"'
Autor:
Sezer, Aytap, Ergin, Tulun, Cesur, Nergis, Tanaka, Shuta J., Kisaka, Shota, Ohira, Yutaka, Yamazaki, Ryo
3C 396 is a composite supernova remnant (SNR), consisting of a central pulsar wind nebula (PWN) and a bright shell in the west, which is known to be interacting with molecular clouds (MCs). We present a study of X-ray emission from the shell and the
Externí odkaz:
http://arxiv.org/abs/1912.08257
We present the results from the Suzaku X-ray Imaging Spectrometer observation of the mixed-morphology supernova remnant (SNR) HB9 (G160.9+2.6). We discovered recombining plasma (RP) in the western Suzaku observation region and the spectra here are we
Externí odkaz:
http://arxiv.org/abs/1907.01017
Akademický článek
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Kes 69 is a mixed-morphology (MM) supernova remnant (SNR) that is known to be interacting with molecular clouds based on 1720 MHz hydroxyl (OH) maser emission observations in the northeastern and southeastern regions. We present an investigation of K
Externí odkaz:
http://arxiv.org/abs/1808.10513
Publikováno v:
Proceedings of the International Astronomical Union, Volume 12, Issue S331, February 2017, pp. 316-319
We investigate the supernova remnant (SNR) 3C 397 and its neighboring pulsar PSR J1906+0722 in high energy gamma rays by using nearly six years of archival data of {\it Large Area Telescope} on board {\it Fermi Gamma Ray Space Telescope} (Fermi-LAT).
Externí odkaz:
http://arxiv.org/abs/1801.05961
A new extended gamma-ray source (PS J1934.5+1845) was detected with a significance of $\sim$13$\sigma$ at a location of 1$^{\circ}\!\!$.83 away from the radio location of the Galactic supernova remnant 3C 400.2 using about 9 years of Fermi-LAT data.
Externí odkaz:
http://arxiv.org/abs/1712.06421
Autor:
Ergin, Tulun, Katsuda, Satoru, Sezer, Aytap, Yamazaki, Ryo, Filipovic, Miroslav, Sano, Hidetoshi, Fukui, Yasuo, Tanaka, Shuta
A new extended gamma-ray source, which was named as Source A, in the southwest of Galactic supernova remnant (SNR) G306.3$-$0.9 was detected with a significance of $\sim$13$\sigma$ at the location of R.A. (J2000) = 13$^{\rm{h}}$ 17$^{\rm{m}}$ 52$^{\r
Externí odkaz:
http://arxiv.org/abs/1712.06415
We present an investigation of the supernova remnant (SNR) G306.3$-$0.9 using archival multi-wavelength data. The Suzaku spectra are well described by two-component thermal plasma models: The soft component is in ionization equilibrium and has a temp
Externí odkaz:
http://arxiv.org/abs/1701.00102
Autor:
Kocaman, Bugra, Harmandali, Murat, Kopru, Mehmet, Solak, Bekir, Ergin, Tulun, Yilmaz, Ercan, Guven, Eylem
Publikováno v:
AIP Conference Proceedings; 2019, Vol. 2178 Issue 1, p030006-1-030006-6, 6p
We have analyzed Chandra X-ray data from different parts of the shell of young supernova remnant (SNR) in the energy range of 0.7 - 8 keV. We observed that X-ray flux level varies over different shell regions of the source. Implications of X-ray obse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=r39c86a4b39b::245078ac8cede3ff6f773e51496cc2d2
https://aperta.ulakbim.gov.tr/record/99673
https://aperta.ulakbim.gov.tr/record/99673