11 citations · 16 across the 5 of their papers we have counts for
6 papers
A study of the composite supernova remnant MSH 15-56 with Suzaku
Nergis Cesur, Aytap Sezer, Jelle de Plaa +1
The Galactic supernova remnant (SNR) MSH 15-56 is a member of the class of composite SNRs that consists of the remnant shell and a displaced pulsar wind nebula (PWN). The earlier X…
Search for the time evolution of the synchrotron X-ray spectrum of the youngest Galactic supernova remnant G1.9+0.3 using Suzaku
A. Sezer, R. Yamazaki, Y. Ohira +2
G1.9+0.3 is the youngest known Galactic supernova remnant (SNR) and dominated by X-ray synchrotron emission. Synchrotron X-rays can be a useful tool to study the electron accelerat…
Detection of an Unidentified Extended Gamma-ray Source Close to the Galactic Supernova Remnant 3C 400.2
Tulun Ergin, Aytap Sezer, Ryo Yamazaki +3
A new extended gamma-ray source (PS J1934.5+1845) was detected with a significance of 13 at a location of 1.83 away from the radio location of the Galactic s…
A New Gamma-Ray Source in the Vicinity of the Galactic Supernova Remnant G306.30.9
Tulun Ergin, Satoru Katsuda, Aytap Sezer +5
A new extended gamma-ray source, which was named as Source A, in the southwest of Galactic supernova remnant (SNR) G306.30.9 was detected with a significance of 13 at t…
Recombining Plasma & Gamma-ray Emission in the Mixed-morphology Supernova Remnant 3C 400.2
T. Ergin, A. Sezer, H. Sano +2
3C 400.2 belongs to the mixed morphology supernova remnant class, showing center-filled X-ray and shell-like radio morphology. We present a study of 3C 400.2 with archival Suzaku a…
The Relation Between the Surface Brightness and the Diameter for Galactic Supernova Remnants
Oktay H. Guseinov, Askin Ankay, Aytap Sezer +1
In this work, we have constructed a relation between the surface brightness () and diameter (D) of Galactic C- and S-type supernova remnants (SNRs). In order to calibrate the $Σ…