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Müller, Simon, Helled, Ravit, Mayer, Lucio (2018) On the Diversity in Mass and Orbital Radius of Giant Planets Formed via Disk Instability. The Astrophysical Journal, 854 (2). 112pp. doi:10.3847/1538-4357/aaa840

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Reference TypeJournal (article/letter/editorial)
TitleOn the Diversity in Mass and Orbital Radius of Giant Planets Formed via Disk Instability
JournalThe Astrophysical Journal
AuthorsMüller, SimonAuthor
Helled, RavitAuthor
Mayer, LucioAuthor
Year2018 (February 16)Volume854
Issue2
PublisherAmerican Astronomical Society
DOIdoi:10.3847/1538-4357/aaa840Search in ResearchGate
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Mindat Ref. ID3545652Long-form Identifiermindat:1:5:3545652:4
GUID0
Full ReferenceMüller, Simon, Helled, Ravit, Mayer, Lucio (2018) On the Diversity in Mass and Orbital Radius of Giant Planets Formed via Disk Instability. The Astrophysical Journal, 854 (2). 112pp. doi:10.3847/1538-4357/aaa840
Plain TextMüller, Simon, Helled, Ravit, Mayer, Lucio (2018) On the Diversity in Mass and Orbital Radius of Giant Planets Formed via Disk Instability. The Astrophysical Journal, 854 (2). 112pp. doi:10.3847/1538-4357/aaa840
In(2018, February) The Astrophysical Journal Vol. 854 (2) American Astronomical Society


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