2006/10/26 by U. Lisenfeld, L. Verdes-Montenegro, L. Verdes‐Montenegro +10 · 4 citations
Engineering · Mathematics · Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Biology #CCD and CMOS Imaging Sensors #Galaxies: Formation, Evolution, Phenomena #Galaxy #Genetics #Geometry #Mathematics #Nature versus nurture #Physics #Point (geometry) #Sample (material) #Universe #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066144
Accepted by A&A, 18 pages, 14 figures. Data of tables 2 and 3 can be obtained from www.iaa.es/AMIGA.html
arxiv created 2006/10/26 · openalex publication_date 2006/11/13 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
Aims.We describe the mid- (MIR) and far- (FIR) infrared properties of a large (~1000) sample of the most isolated galaxies in the local Universe. This sample is intended as a “nurture-free” zero point against which more environmentally influenced samples can be compared.