2007/03/28 by R. Szczerba, N. Siódmiak, N. Siodmiak +3 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Galactic nuclei #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Infrared #Sensitivity (control systems) #Sky #Stars #Stellar, planetary, and galactic studies #Ultraviolet astronomy #astro-ph
paper · pdf · doi:10.1051/0004-6361:20067035
9 pages, 6 figures, accepted for publication in A&A
arxiv created 2007/03/28 · openalex publication_date 2007/03/29 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims.With the ongoing AKARI infrared sky survey, of much greater sensitivity than IRAS, a wealth of post-AGB objects may be discovered. It is thus time to organize our present knowledge of known post-AGB stars in the galaxy with a view to using it to search for new post-AGB objects among AKARI sources.