Mallory S. E. Roberts

TL;DR: In this article, the authors investigated the mechanism by which supernova ejected stars were ejected from their parent open cluster, NGC 654, and presented the results of a radio pulsar search of these systems, as well as estimates of their predicted X-ray flux assuming that each binary contains a compact object.

TL;DR: A remarkable number of pulsar wind nebulae (PWN) are coincident with EGRET γ-ray sources and their toroidal morphologies can help determine the geometry of the pulsar as discussed by the authors.

TL;DR: In this article, the authors reported the discovery of a partial 2° diameter nonthermal radio shell coincident with Taz, the pulsar wind nebula (PWN) in the error box of the apparently variable γ-ray source 3EG J1809−2328.

TL;DR: The Green Bank North Celestial Cap (GBNCC) pulsar survey is one of the most uniform and sensitive all-sky surveys to date as discussed by the authors, and the authors of this paper present measured signal-to-noise ratios (S/N), flux densities, pulse widths, profiles, and where appropriate, refined measurements of dispersion measures (DMs) and new or improved spectral indices.

TL;DR: In this article, the authors derived a lower distance limit of 6 kpc to the supernova remnant (SNR) G312.4-0.4 and the two young pulsars PSRs J1412-6145 and J1413-6141.