Radiation thermo-chemical models of protoplanetary disks
نویسندگان
چکیده
منابع مشابه
Chemical Models of the Protoplanetary Disks for Extrasolar Planetary
Introduction: It is widely known that extrasolar planetary host stars are, to some degree, chemically anomalous. Spectroscopic studies of these stars have revealed that the metallicity of the host star is higher than that of other F, G and K type stars not known to harbor planetary companions (e.g. [1-3]). Trends may also exist in the abundance of Li, C, N, [4] Na, Mg and Al [5]. One aspect of ...
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3 Material Inventory and Fundamental Chemical Processes in Disks 14 3.1 Inventory of Gas-Phase Molecules . . . . . . . . . . . . . . . . . . . . . . . . . . 14 3.1.1 Results from (Sub-)millimeter Spectroscopy . . . . . . . . . . . . . . . . . 15 3.1.2 Results from Far-Infrared Spectroscopy . . . . . . . . . . . . . . . . . . . 17 3.1.3 Results from Midand Near-Infrared Spectroscopy . . . . . . ...
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ژورنال
عنوان ژورنال: Astronomy and Astrophysics
سال: 2010
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/200913076