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نپتون داغ (Persian Wikipedia)

Analysis of information sources in references of the Wikipedia article "نپتون داغ" in Persian language version.

refsWebsite
Global rank Persian rank
2arxiv.org
69th place
253rd place
2doi.org
2nd place
2nd place
2web.archive.org
1st place
1st place
2cosis.net
low place
low place
2nih.gov
4th place
5th place
1harvard.edu
18th place
50th place

arxiv.org

  • Dong (23 June 2017). "LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements". Proceedings of the National Academy of Sciences. 115 (2): 266–271. arXiv:1706.07807. doi:10.1073/pnas.1711406115. PMC 5777037. PMID 29284755. {{cite journal}}: Unknown parameter |displayauthors= ignored (|display-authors= suggested) (help)
  • D'Angelo, G.; Bodenheimer, P. (2016). "In Situ and Ex Situ Formation Models of Kepler 11 Planets". The Astrophysical Journal. 828 (1): id. 33. arXiv:1606.08088. Bibcode:2016ApJ...828...33D. doi:10.3847/0004-637X/828/1/33.

cosis.net

  • G. Wuchterl. "Hot Neptunes: A Key To Giant Planet Formation" (PDF). Archived from the original (PDF) on 17 June 2019. Retrieved 3 August 2015. {{cite journal}}: Cite journal requires |journal= (help)
  • «Oligarchic formation of hot Neptunes» (PDF). بایگانی‌شده از اصلی (PDF) در ۶ اكتبر ۲۰۱۷. دریافت‌شده در ۳ ژوئن ۲۰۲۳. تاریخ وارد شده در |archive-date= را بررسی کنید (کمک)

doi.org

  • Dong (23 June 2017). "LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements". Proceedings of the National Academy of Sciences. 115 (2): 266–271. arXiv:1706.07807. doi:10.1073/pnas.1711406115. PMC 5777037. PMID 29284755. {{cite journal}}: Unknown parameter |displayauthors= ignored (|display-authors= suggested) (help)
  • D'Angelo, G.; Bodenheimer, P. (2016). "In Situ and Ex Situ Formation Models of Kepler 11 Planets". The Astrophysical Journal. 828 (1): id. 33. arXiv:1606.08088. Bibcode:2016ApJ...828...33D. doi:10.3847/0004-637X/828/1/33.

harvard.edu

ui.adsabs.harvard.edu

nih.gov

ncbi.nlm.nih.gov

  • Dong (23 June 2017). "LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements". Proceedings of the National Academy of Sciences. 115 (2): 266–271. arXiv:1706.07807. doi:10.1073/pnas.1711406115. PMC 5777037. PMID 29284755. {{cite journal}}: Unknown parameter |displayauthors= ignored (|display-authors= suggested) (help)

pubmed.ncbi.nlm.nih.gov

  • Dong (23 June 2017). "LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements". Proceedings of the National Academy of Sciences. 115 (2): 266–271. arXiv:1706.07807. doi:10.1073/pnas.1711406115. PMC 5777037. PMID 29284755. {{cite journal}}: Unknown parameter |displayauthors= ignored (|display-authors= suggested) (help)

web.archive.org

  • G. Wuchterl. "Hot Neptunes: A Key To Giant Planet Formation" (PDF). Archived from the original (PDF) on 17 June 2019. Retrieved 3 August 2015. {{cite journal}}: Cite journal requires |journal= (help)
  • «Oligarchic formation of hot Neptunes» (PDF). بایگانی‌شده از اصلی (PDF) در ۶ اكتبر ۲۰۱۷. دریافت‌شده در ۳ ژوئن ۲۰۲۳. تاریخ وارد شده در |archive-date= را بررسی کنید (کمک)