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20032026
most citedRecombining Plasma & Gamma-ray Emission in the Mixed-morphology Supernova Remnant 3C 400.2

11 citations · 20 across the 10 of their papers we have counts for

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astro-ph.HE2026

Optical observations and atomic environment of supernova remnant G25.1-2.3

Ebru Aktekin, Hicran Bakış, Volkan Bakış +4

The supernova remnant (SNR) G25.1-2.3 was identified in the radio band during the Sino-German 6 cm survey of the Galactic plane. We present a detailed investigation of the optic…

astro-ph.HE2026

First detailed optical spectroscopic observations of the supernova remnants G107.7-5.1 and G150.3+4.5

Ebru Aktekin, Hicran Bakış, Volkan Bakış +1

We present optical spectroscopic observations of the supernova remnants (SNRs) G107.75.1 and G150.3+4.5, each spanning nearly 3 degree. Both remnants were recently examined in t…

astro-ph.HE2025

Optical investigation of supernova remnant G206.7+5.9

Hicran Bakis, Ebru Aktekin, Volkan Bakis +2

The shell-type supernova remnant (SNR) G206.7+5.9 was recently discovered in the radio band with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The remnant spans…

astro-ph.HE2024

Optical and HI observations of IC 443 and G189.6+3.3 in a complex environment

Hicran Bakis, Gunay Payli, Ebru Aktekin +2

The supernova remnant (SNR) IC 443 is one of the best-studied Galactic SNRs at many wavelengths. It is interacting with a very complex environment, including the SNR G189.6+3.3 and…

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.HE2019

Discovery of recombining plasma inside the extended gamma-ray supernova remnant HB9

Aytap Sezer, Tulun Ergin, Ryo Yamazaki +2

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…