2008/04/21 by A. J. Dean, A. B. Hill · 4 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Binary pulsar #Nebula #Pulsar #Pulsar planet #Pulsar wind nebula #Pulsars and Gravitational Waves Research #Scientific Research and Discoveries #X-ray pulsar #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809356
published in Astronomy and Astrophysics 485(1), 195-198 (EDP Sciences) · 4 pages, 1 figure, accepted for publication as a Research Note in Astronomy & Astrophysics
arxiv created 2008/04/21 · openalex publication_date 2008/04/22 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. We investigate the possible theoretical properties of the putative pulsar associated with the pulsar wind nebula IGR J18135-1751/HESS J1813-178 based upon recent γ-ray observations and archival multi-wavelength observations.