Spectrophotometry of the Orion Nebula. II. The abundance of elements

Details Spectrophotometry of the Orion Nebula. II. The abundance of elements Spectrophotometry of the Orion Nebula. II. The abundance of elements

Oct 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968bott....4..240m&link_type=abstract

Boletín de los Observatorios de Tonantzintla y Tacubaya Vol. 4, pp. 240-245 (1968) (http://www.astroscu.unam.mx/bott/)

Astronomy and Astrophysics

Astronomy

3

Ism: Abundances, Hii Regions, Photometry

Scientific paper

Using a recent spectrophotometric study of the Orion Nebula, the
chemical composition of this object is derived. The electron temperature
is also given. The abundance by mass is X = 0.713; Y = 0.26 +/- 0.02; Z
= 0.027 +/- 0.004, which is very close to the so-called primordial
abundance.

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