Stanley, Sabine; Bloxham, Jeremy. Convective-region geometry as the cause of Uranus' and Neptune's unusual magnetic fields. Letters to Nature. 2004, 428: 151–153. PMID 15014493. doi:10.1038/nature02376.引文使用过时参数coauthors (帮助)
Podolak, M.; Weizman, A.; Marley, M. Comparative model of Uranus and Neptune. Planet. Space Sci. 1995, 43 (12): 1517–1522 [2007-10-14]. (原始内容存档于2007-10-11).引文使用过时参数coauthors (帮助)
Feuchtgruber, H.; Lellouch, E.; Bézard, B.; Encrenaz, Th.; de Graauw, Th.; Davis, G. R. Detection of HD in the atmospheres of Uranus and Neptune: a new determination of the D/H ratio. Astronomy and Astrophysics. 1999, 341: L17–L21. Bibcode:1999A&A...341L..17F.
Stanley, Sabine; Bloxham, Jeremy. Convective-region geometry as the cause of Uranus' and Neptune's unusual magnetic fields. Letters to Nature. 2004, 428: 151–153. PMID 15014493. doi:10.1038/nature02376.引文使用过时参数coauthors (帮助)
Podolak, M.; Weizman, A.; Marley, M. Comparative model of Uranus and Neptune. Planet. Space Sci. 1995, 43 (12): 1517–1522 [2007-10-14]. (原始内容存档于2007-10-11).引文使用过时参数coauthors (帮助)