2006/12/31 by M. Pena, María Teresa Cuamatzi Peña, M. G. Richer +2
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Doubly ionized oxygen #Emission nebula #Emission spectrum #Galaxies: Formation, Evolution, Phenomena #Galaxy #Line (geometry) #Luminosity #Nebula #Physics #Planetary nebula #Population #Spectral line #Star formation #Stars #Stellar population #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066675
8 pages, including 4 figures and 3 tables. Accepted in A&A. Replaced with the final version
openalex publication_date 2007/01/29 · arxiv created 2007/01/30 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims.Images obtained with the ESO VLT and FORS1 in [O iii] 5007 on- and off-band, as well as rGunn filters, are analyzed to search for planetary nebula (PN) candidates.