AN ABUNDANCE COMPARISON BETWEEN B STARS AND NEBULA IN THE ORION ASSOCIATION

Authors
CUNHA K
Citation
K. Cunha, AN ABUNDANCE COMPARISON BETWEEN B STARS AND NEBULA IN THE ORION ASSOCIATION, Revista Mexicana de Astronomia y Astrofisica, 27, 1993, pp. 111-114
Citations number
16
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Revista Mexicana de Astronomia y Astrofisica → ACNP
ISSN journal
01851101
Volume
27
Year of publication
1993
Pages
111 - 114
Database
ISI
SICI code
0185-1101(1993)27:<111:AACBBS>2.0.ZU;2-0
Abstract
LTE Carbon, Nitrogen and Oxygen abundances are presented for 12 B star s belonging to the youngest subgroups of the Orion association. These stellar analyses confirm published abundances analyses of the Orion Ne bula that show Orion to be underabundant relative to the Sun.