Rujukan Gergasi_gas

  1. 1 2 The Interior of Jupiter, Guillot et al., in Jupiter: The Planet, Satellites and Magnetosphere, Bagenal et al., editors, Cambridge University Press, 2004
  2. 1 2 Burgasser, A. J. (June 2008). "Brown dwarfs: Failed stars, super Jupiters" (PDF). Physics Today. Dicapai 11 January 2016. 
  3. ↑ Science Fiction Citations, Citations for gas giant n.
  4. 1 2 D'Angelo, G.; Durisen, R. H.; Lissauer, J. J. (2011). "Giant Planet Formation". dalam S. Seager. Exoplanets. University of Arizona Press, Tucson, AZ. m/s. 319–346. arXiv:1006.5486 . Bibcode:2010exop.book..319D. 
  5. ↑ Science Fiction Citations, Citations for gas giant n.
  6. 1 2 Seager, S.; Kuchner, M.; Hier-Majumder, C. A.; Militzer, B. (2007). "Mass-Radius Relationships for Solid Exoplanets". The Astrophysical Journal. 669 (2): 1279–1297. arXiv:0707.2895 . Bibcode:2007ApJ...669.1279S. doi:10.1086/521346. 
  7. ↑ Patrick G. J. Irwin (2003). Giant Planets of Our Solar System: Atmospheres, Composition, and Structure. Springer. ISBN 3-540-00681-8. 
  8. ↑ "Class 12 – Giant Planets – Heat and Formation". 3750 – Planets, Moons & Rings. Colorado University, Boulder. 2004. Dicapai 2008-03-13. 
  9. ↑ Feng Tian; Toon, Owen B.; Pavlov, Alexander A.; De Sterck, H. (March 10, 2005). "Transonic hydrodynamic escape of hydrogen from extrasolar planetary atmospheres". The Astrophysical Journal. 621: 1049–1060. Bibcode:2005ApJ...621.1049T. CiteSeerX 10.1.1.122.9085 . doi:10.1086/427204. 
  10. ↑ Mass-radius relationships for exoplanets, Damian C. Swift, Jon Eggert, Damien G. Hicks, Sebastien Hamel, Kyle Caspersen, Eric Schwegler, and Gilbert W. Collins
  11. ↑ Three regimes of extrasolar planets inferred from host star metallicities, Buchhave et al.
  12. ↑ Earth-mass exoplanet is no Earth twin – Gaseous planet challenges assumption that Earth-mass planets should be rocky
  13. ↑


Rujukan

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