2008/06/17 by G. Dubner, Gloria Dubner, E. Giacani +3
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #Crab Nebula #High resolution #Near-Earth supernova #Nebula #Pulsar #Pulsar wind nebula #Pulsars and Gravitational Waves Research #Supernova remnant #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809987
10 pages,8 figures, accepted for publication in A&A, June 13 2008
arxiv created 2008/06/17 · openalex publication_date 2008/06/24 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims. We have conducted a study in radio wavelengths and in X-rays of the pulsar wind nebula (PWN) in the supernova remnant (SNR) G0.9+0.1 with the goal of investigating in detail its morphology and to accurately determine its characteristic parameters.