A simple way to model nebulae with distributed ionizing stars
- Author
- JAMET, L1 ; MORISSET, C1
[1] Instituto de Astronomfa, Universidad Nacional Autónoma de México, Apartado Postal 70-264, Ciudad Universitaria, México D.F. 04510, Mexico - Source
Astronomy and astrophysics (Berlin. Print). 2008, Vol 482, Num 1, pp 209-214, 6 p ; ref : 1/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- ISM: HII regions ISM: abundances stars: abundances
- Keyword (fr)
- Abondance stellaire Age Etoile excitatrice Ionisation Modèle Métallicité Photoionisation Population stellaire Région HII Répartition spatiale Spectre émission Sphère
- Keyword (en)
- Stellar abundance Age Exciting star Ionization Models Metallicity Photoionization Stellar population HII regions Spatial distribution Emission spectra Spheres
- Keyword (es)
- Abundancia estelar Edad Estrella excitadora Modelo Metalicidad Población estelar
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20262852
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1051/0004-6361:20078606 
https://dx.doi.org/10.1051/0004-6361:20078606
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