Molecular hydrogen emission from protoplanetary disks. II. Effects of X-ray irradiation and dust evolution
- Author
- NOMURA, H1 2 ; AIKAWA, Y1 ; TSUJIMOTO, M3 ; NAKAGAWA, Y1 ; MILLAR, T. J2
[1] Department of Earth and Planetary Sciences, Kobe University, Nada, Kobe 657-8501, Japan
[2] Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, Northern Ireland, United Kingdom
[3] Department ofPhysics, Rikkyo University, Toshima, Tokyo 171-8501, Japan - Source
The Astrophysical journal. 2007, Vol 661, Num 1, pp 334-353, 20 p ; 1 ; ref : 1 p.1/4
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- line: formation molecular processes planetary systems: protoplanetary disks radiative transfer
- Keyword (fr)
- Formation raie Hydrogène molécule Irradiation RX Nébuleuse proto planétaire Processus moléculaire Système planétaire Transfert radiatif
- Keyword (en)
- Line formation Hydrogen molecules X ray irradiation Proto planetary nebula Molecular process Planetary system Radiative transfer
- Keyword (es)
- Irradiación RX Nebulosa proto planetaria Proceso molecular Sistema planetario
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18782467
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
10.1086/513419 
https://dx.doi.org/10.1086/513419
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