2014/06/16 by X. Y. Gao, J. L. Han
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Cosmic Phenomena #Gamma-ray bursts and supernovae #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201424128
published as A&A 567, A59 (2014) · 5 pages, 3 figures, accepted for publication of Astronomy and Astrophysics
arxiv created 2014/06/16 · openalex publication_date 2014/06/18 · arxiv updated 2014/09/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. Large-scale radio continuum surveys have good potential for discovering new Galactic supernova remnants (SNRs). Surveys of the Galactic plane are often limited in the Galactic latitude of | b | ~ 5°. SNRs at high latitudes, such as the Cygnus Loop or CTA 1, cannot be detected by surveys in such limited latitudes.