2006/11/20 by G. Trinchieri, D. Breitschwerdt, W. Pietsch +3 · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Geology #History #Morphology (biology) #Paleontology #Physics #ROSAT #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066156
Accepted for pubblication in Astronomy & Astrophysics. Figs 1, 2, 3 and 9-12 are given as JPEG files due to the restrictions on space available on astro-ph
arxiv created 2006/11/20 · openalex publication_date 2006/11/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims.A peculiar morphology of the hot gas was discovered at the center of IC 1262 with the ROSAT HRI. Sensitive Chandra and XMM-Newton data were requested to investigate the characteristics of this structure to understand its nature.