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Volumn 321, Issue 5890, 2008, Pages 814-817

Gas disks to gas giants: Simulating the birth of planetary systems

Author keywords

[No Author keywords available]

Indexed keywords

GAS; NUMERICAL MODEL; PLANET; SOLAR SYSTEM;

EID: 49449090903     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1159723     Document Type: Article
Times cited : (139)

References (41)
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    • disk, thus making substantial migration likely in all planetary systems.
    • disk, thus making substantial migration likely in all planetary systems.
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    • We thank the Spitzer Space Telescope Cycle-4 Theoretical Research Program, NSF, and the Natural Sciences and Engineering Research Council of Canada for supporting this work, and two anonymous referees for valuable comments
    • We thank the Spitzer Space Telescope Cycle-4 Theoretical Research Program, NSF, and the Natural Sciences and Engineering Research Council of Canada for supporting this work, and two anonymous referees for valuable comments.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.