PMO OpenIR
volatiledepletioninplanetformingdisks
Du Fujun
2020
Source Publicationchinesejournalofchemicalphysics
ISSN1674-0068
Volume33Issue:1Pages:85
AbstractNewly born stars are surrounded by gas and dust with a flattened axisymmetric distribution termed protoplanetary disk, in which planets are formed. Observations of these objects are necessary for understanding the formation and early evolution of stars and planets, and for revealing the composition of the raw material from which planets are made. Numerical models can extract important parameters from the observational data, including the gas and dust mass of the disk. These parameters are used as input for further modeling, e.g., to calculate the chemical composition of the disk. A consistent thermochemical model should be able to reproduce the abundances of different species in the disk. However, this good wish has been challenged for many disks: models over-predict the emission line intensity of some species; namely, they are depleted(with respect to expectations from canonical models). In this review we show how this disparity indicates that dust evolution has significant effects on gas chemistry, and may indicate the earliest stages of planet formation.
Language英语
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/35784
Collection中国科学院紫金山天文台
Affiliation中国科学院紫金山天文台
First Author Affilication中国科学院紫金山天文台
Recommended Citation
GB/T 7714
Du Fujun. volatiledepletioninplanetformingdisks[J]. chinesejournalofchemicalphysics,2020,33(1):85.
APA Du Fujun.(2020).volatiledepletioninplanetformingdisks.chinesejournalofchemicalphysics,33(1),85.
MLA Du Fujun."volatiledepletioninplanetformingdisks".chinesejournalofchemicalphysics 33.1(2020):85.
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