An article accepted for publication in “The Astrophysical Journal” reports a study on the long filament generated by the pulsar cataloged as PSR J2030+4415, or simply J2030. Martjin de Vries and Roger Romani of the American Stanford University used observations made using NASA’s Chandra X-ray Observatory and ground-based telescopes to study a filament that has an estimated length of about 7 light-years and is composed of matter but also of antimatter. Pulsar emissions of this type could explain positron detections in the Milky Way.