activity
20152019
most citedPulsar Wind Nebulae Created by Fast-Moving Pulsars

84 citations · 180 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2019

Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur revisited

Blagoy Rangelov, Thierry Montmerle, S. R. Federman +2

We present results of our Chandra/ACIS observations of the field centered on the fast, runaway O star AE Aur and its bow shock. Previous XMM-Newton observations revealed an X-ray "…

astro-ph.HE20194 cited

XMM-Newton and Chandra observations of the unidentified Fermi-LAT source 3FGL J1016.5-6034: A Young Pulsar with a Nebula?

Jeremy Hare, Igor Volkov, Oleg Kargaltsev +2

We report the discovery of a bright X-ray source in the XMM-Newton and Chandra X-ray Observatory (CXO) images of the unidentified Fermi-LAT source 3FGL J1016.5-6034. The XMM-Newton…

astro-ph.HE201951 cited

Hubble Space Telescope non-detection of PSR J2144-3933: the coldest known neutron star

S. Guillot, G. G. Pavlov, C. Reyes +4

We report non-detections of the yr old, slow, isolated, rotation-powered pulsar PSR J21443933 in observations with the Hubble Space Telescope in one optical…

astro-ph.HE2018

A long hard-X-ray look at the dual active galactic nuclei of M51 with NuSTAR

M. Brightman, M. Baloković, M. Koss +14

We present a broadband X-ray spectral analysis of the M51 system, including the dual active galactic nuclei (AGN) and several off-nuclear point sources. Using a deep observation by…

astro-ph.HE201741 cited

Old but still warm: Far-UV detection of PSR B0950+08

G. G. Pavlov, B. Rangelov, O. Kargaltsev +3

We report on a Hubble Space Telescope detection of the nearby, old pulsar B0950+08 ( pc, spin-down age 17.5 Myr) in two far-ultraviolet (FUV) bands. We measured the me…

astro-ph.HE201784 cited

Pulsar Wind Nebulae Created by Fast-Moving Pulsars

Oleg Kargaltsev, George G. Pavlov, Noel Klingler +1

We review multiwavelength properties of pulsar wind nebulae (PWNe) created by supersonically moving pulsars and the effects of pulsar motion on the PWN morphologies and the ambient…