activity
19952020
most citedCooling neutron stars and superfluidity in their interiors

276 citations · 598 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2020★ 116 cited

Thermal luminosities of cooling neutron stars

A. Y. Potekhin, D. A. Zyuzin, D. G. Yakovlev +2

Ages and thermal luminosities of neutron stars, inferred from observations, can be interpreted with the aid of the neutron star cooling theory to gain information on the properties…

astro-ph.HE2020★ 15 cited

Atacama Compact Array Observations of the Pulsar-Wind Nebula of SNR 0540-69.3

P. Lundqvist, N. Lundqvist, C. Vlahakis +6

We present observations of the pulsar-wind nebula (PWN) region ofSNR 0540-69.3. The observations were made with the Atacama Compact Array (ACA) in Bands 4 and 6. We also add radio…

astro-ph.HE2020★ 3 cited

Studying the -ray pulsar J1932+1916 and its pulsar wind nebula with Chandra

O. D. Medvedev, A. V. Karpova, Yu. A. Shibanov +2

We report on the results of Chandra X-ray observations of the -ray radio-quiet pulsar J1932+1916. We confirm the previous detection of the pulsar counterpart and its pulsar wind…

astro-ph.SR2018★ 4 cited

Optical identification of the millisecond pulsar J0621+2514

A. V. Karpova, D. A. Zyuzin, Yu. A. Shibanov +2

Using the SDSS and Pan-STARRS1 survey data, we found a likely companion of the recently discovered binary -ray radio-loud millisecond pulsar J0621+2514. Its visual brightness is…

astro-ph.SR2013★ 15 cited

The PSR J1124-5916 wind nebula in the near-infrared

Sergey V. Zharikov, Dmitry A. Zyuzin, Yuri A. Shibanov +1

The young radio pulsar J1124-5916 is associated with a Cas A like supernova remnant G292.0+1.8. It powers a compact torus-like pulsar wind nebula with a jet first detected in X-ray…

astro-ph.HE2011★ 38 cited

The Young Pulsar J1357-6429 and Its Pulsar Wind Nebula

Chulhoon Chang, George G. Pavlov, Oleg Kargaltsev +1

We observed the young pulsar J1357--6429 with the {\it Chandra} and {\it XMM-Newton} observatories. The pulsar spectrum fits well a combination of absorbed power-law model ($Γ=1.7\…