Computer Science
Scientific paper
Sep 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982msngr..29...18c&link_type=abstract
The Messenger, No.29, P. 18, 1982
Computer Science
Scientific paper
The determination of abundances in planetary nebulae (PN) and H 11
regions is important for studying the present and past chemical
composition of galaxies. Its derivation from the spectral-Iine
intensities involves basically the following steps:
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