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Թեժ Նեպտուն կամ Հոպտուն (Armenian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Թեժ Նեպտուն կամ Հոպտուն" in Armenian language version.

refsWebsite
Global rank Armenian rank
6arxiv.org
69th place
186th place
4doi.org
2nd place
4th place
4harvard.edu
18th place
38th place
2web.archive.org
1st place
1st place
2cosis.net
low place
low place
2nih.gov
4th place
3rd place
1caltech.edu
887th place
416th place
1arizona.edu
1,592nd place
919th place
1phys.org
1,283rd place
561st place

arizona.edu

uapress.arizona.edu

arxiv.org

  • Dong; և այլք: (2017 թ․ հունիսի 23). «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.
  • 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.{{cite journal}}: CS1 սպաս․ չպիտակված ազատ DOI (link)
  • Adrián Brunini and Rodolfo G. Cionco (September 2005). «The origin and nature of Neptune-like planets orbiting close to solar type stars». Icarus. 177 (1): 264–68. arXiv:astro-ph/0511051. Bibcode:2005Icar..177..264B. doi:10.1016/j.icarus.2005.02.015.
  • D'Angelo, G.; Durisen, R. H.; Lissauer, J. J. (2011). «Giant Planet Formation». In S. Seager. (ed.). Exoplanets. University of Arizona Press, Tucson, AZ. էջեր 319–346. arXiv:1006.5486. Bibcode:2010exop.book..319D.
  • D'Angelo, G.; Lissauer, J. J. (2018). «Formation of Giant Planets». In Deeg H., Belmonte J. (ed.). Handbook of Exoplanets. Springer International Publishing AG, part of Springer Nature. էջեր 2319–2343. arXiv:1806.05649. Bibcode:2018haex.bookE.140D. doi:10.1007/978-3-319-55333-7_140. ISBN 978-3-319-55332-0.
  • An Ultra-Hot Neptune in the Neptune desert, James S. Jenkins et al, 27 Sep 2020

caltech.edu

exoplanetarchive.ipac.caltech.edu

cosis.net

doi.org

  • Dong; և այլք: (2017 թ․ հունիսի 23). «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.
  • 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.{{cite journal}}: CS1 սպաս․ չպիտակված ազատ DOI (link)
  • Adrián Brunini and Rodolfo G. Cionco (September 2005). «The origin and nature of Neptune-like planets orbiting close to solar type stars». Icarus. 177 (1): 264–68. arXiv:astro-ph/0511051. Bibcode:2005Icar..177..264B. doi:10.1016/j.icarus.2005.02.015.
  • D'Angelo, G.; Lissauer, J. J. (2018). «Formation of Giant Planets». In Deeg H., Belmonte J. (ed.). Handbook of Exoplanets. Springer International Publishing AG, part of Springer Nature. էջեր 2319–2343. arXiv:1806.05649. Bibcode:2018haex.bookE.140D. doi:10.1007/978-3-319-55333-7_140. ISBN 978-3-319-55332-0.

harvard.edu

ui.adsabs.harvard.edu

nih.gov

ncbi.nlm.nih.gov

  • Dong; և այլք: (2017 թ․ հունիսի 23). «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.

pubmed.ncbi.nlm.nih.gov

  • Dong; և այլք: (2017 թ․ հունիսի 23). «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.

phys.org

web.archive.org