Molecular Distributions in the Inner Regions of Protostellar Disks
| Data(s) |
01/04/2002
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|---|---|
| Resumo |
The distributions of molecules in the inner regions of a protostellar disk are presented. These were calculated using an uncoupled chemical/dynamical model, with a numerical integration of the vertical disk structure. A comparison between models with and without the effects of X-ray ionisation is made, and molecules are identified which are good tracers of the ionisation level in this part of the disk, notably CN and C_2H. In the region considered in this paper (r |
| Identificador |
http://dx.doi.org/10.1051/0004-6361:20020050 http://www.scopus.com/inward/record.url?scp=0036530802&partnerID=8YFLogxK |
| Idioma(s) |
eng |
| Direitos |
info:eu-repo/semantics/restrictedAccess |
| Fonte |
Millar , T J , Markwick , A J , Illgner , M & Henning , T 2002 , ' Molecular Distributions in the Inner Regions of Protostellar Disks ' Astronomy and Astrophysics , vol 385 , no. 2 , pp. 632-646 . DOI: 10.1051/0004-6361:20020050 |
| Palavras-Chave | #/dk/atira/pure/subjectarea/asjc/1900/1912 #Space and Planetary Science |
| Tipo |
article |
