Temperature variations and n+/o+ in the orion nebula II the collision strengths

We continue an investigation of electron temperature (Te), mean{square Tevariation (t2), and the N+/O+ abundance ratio. Our previous analysis of HSTspectra of the Orion Nebula used collision strengths for N+ by Sta ord et al. (1994).Here we examine the consequences of changing just these collision s...

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發表在:Revista Mexicana de Astronomía y Astrofísica
Main Authors: R. H. Rubin, R. J. Dufour, P. G. Martin, G. J. Ferland, J. A. Baldwin, C. O. Ortiz, D. K. Walter
格式: Artigo
語言:Inglês
出版: Universidad Nacional Autónoma de México 2001
主題:
Física, Astronomía y Matemáticas
ISM: IN
ISM: ABUNDANCES
ISM: H II REGIONS
DIVIDUAL: ORION NEBULA
在線閱讀:https://www.redalyc.org/articulo.oa?id=57101008
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