output
20162023
most citedRecombining Plasma & Gamma-ray Emission in the Mixed-morphology Supernova Remnant 3C 400.2

11 citations

Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE20236 cited

Discovery of optical emission associated with the supernova remnant G107.5-1.5

Hicran Bakis, Gunay Bulut, Volkan Bakis +2

We present the first results from an imaging and a spectroscopic survey of the optical emission associated with supernova remnant (SNR) G107.51.5. We discovered optical diffuse…

astro-ph.HE20194 cited

Suzaku and Fermi view of the supernova remnant 3C 396

Aytap Sezer, Tulun Ergin, Nergis Cesur +4

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 clou…

astro-ph.HE20195 cited

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…

astro-ph.HE2017

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…

astro-ph.HE201711 cited

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…

astro-ph.HE20168 cited

Suzaku Analysis of the Supernova Remnant G306.3-0.9 and the Gamma-ray View of Its Neighborhood

Aytap Sezer, Tulun Ergin, Ryo Yamazaki

We present an investigation of the supernova remnant (SNR) G306.30.9 using archival multi-wavelength data. The Suzaku spectra are well described by two-component thermal plasma…