activity
20142017
most citedThermal properties of the middle-aged pulsar J1741-2054

16 citations · 52 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2017★ 2 cited

Proper motion of the radio pulsar B1727-47 and its association with the supernova remnant RCW 114

P. Shternin, M. Yu, A. Kirichenko +4

We report preliminary results of the analysis of the proper motion of the bright radio pulsar B172747. Using archival Parkes timing data, as well as original and archival ATCA i…

astro-ph.HE2016★ 9 cited

Observations of the -ray pulsar J1932+1916 in X-rays

A. Karpova, P. Shternin, D. Zyuzin +2

We present the analysis of the archival Suzaku and Swift X-ray observations of the young -ray pulsar J1932+1916 field. The data revealed a point-like object at the -ray posit…

astro-ph.SR2016★ 6 cited

XMM-Newton Studies of the Supernova Remnant G350.02.0

A. Karpova, P. Shternin, D. Zyuzin +2

We report the results of XMM-Newton observations of the Galactic mixed-morphology supernova remnant G350.02.0. Diffuse thermal X-ray emission fills the north-western part of the…

astro-ph.HE2015★ 14 cited

Constraining the parameters of the pulsar wind nebula DA 495 and its pulsar with Chandra and XMM-Newton

A. Karpova, D. Zyuzin, A. Danilenko +1

We present spectral and timing analyses of the X-ray emission from the pulsar wind nebula DA 495 and its central object, J1952.2+2925, suggested to be the pulsar, using archival Ch…

astro-ph.SR2015★ 5 cited

Observations of PSR J1357-6429 at 2.1 GHz with the Australia Telescope Compact Array

A. Kirichenko, Yu. Shibanov, P. Shternin +6

PSR J13576429 is a young and energetic radio pulsar detected in X-rays and -rays. It powers a compact pulsar wind nebula with a jet visible in X-rays and a large scale plerio…

astro-ph.SR2014★ 16 cited

Thermal properties of the middle-aged pulsar J1741-2054

A. Karpova, A. Danilenko, Yu. Shibanov +2

We present results of the spectral analysis of the X-ray emission from the middle-aged Fermi pulsar J17412054 using all Chandra archival data collected in 2010 and 2013. We conf…