プロキシマ・ケンタウリ (Japanese Wikipedia)

Analysis of information sources in references of the Wikipedia article "プロキシマ・ケンタウリ" in Japanese language version.

refsWebsite
Global rank Japanese rank
18th place
107th place
2nd place
6th place
69th place
227th place
5th place
19th place
3,034th place
4,779th place
4th place
24th place
75th place
171st place
1st place
1st place
234th place
363rd place
936th place
1,733rd place
6th place
146th place
896th place
2,100th place
9,995th place
8,815th place
3rd place
61st place
1,342nd place
415th place
low place
5,729th place
low place
4,760th place
low place
low place
1,725th place
2,169th place
769th place
6,616th place
7th place
63rd place
30th place
177th place
low place
low place
low place
low place
1,349th place
3,050th place
916th place
2,207th place
857th place
1,005th place
low place
low place
low place
low place
145th place
10th place
low place
low place
6,724th place
9,773rd place
low place
low place
993rd place
2,074th place
low place
1,577th place
466th place
747th place
657th place
1,487th place
1,985th place
1,575th place
2,691st place
1,320th place

archive.org

  • Go to WayBackMachine INTERNET ARCHIVE. Enter http://www.eso.org/outreach/press-rel/pr-2002/pr-22-02.html. Choose 20 August 2006 for ESO Press Release: "How Small are Small Stars Really?".
  • Go to WayBackMachine INTERNET ARCHIVE. Enter http://www.eso.org/outreach/press-rel/pr-2002/pr-22-02.html. Choose 20 August 2006 for ESO Press Release: "How Small are Small Stars Really?"

arxiv.org

astroarts.com

astrobiology.com

books.google.com

  • 天頂の南にある恒星の場合、天頂に対する角度は緯度から赤緯を引いたものに等しくなる。天頂角が90°以上、つまり地平線より下になると恒星は見えなくなる。プロキシマ・ケンタウリの場合は以下のようになる。
    Highest latitude = 90° + −62.68° = 27.32°.
    以下も参照。

centauri-dreams.org

doi.org

earthsky.org

engadget.com

japanese.engadget.com

eso.org

exoplanet.eu

exoplanetkyoto.org

harvard.edu

ui.adsabs.harvard.edu

chandra.harvard.edu

iau.org

illinois.edu

stars.astro.illinois.edu

  • Kaler, Jim. “Rigil Kentaurus”. University of Illinois. 2016年8月26日閲覧。

inta-csic.es

sdc.cab.inta-csic.es

iop.org

iopscience.iop.org

msu.su

sai.msu.su

  • GCVS”. Results for V645 Cen. 2016年8月27日閲覧。

nasa.gov

solarsystem.nasa.gov

  • 密度(ρ)は質量と体積より求める事ができる。したがって、太陽を基準とした密度は次のようになる。
    =
    = 0.123 · 0.145-3 · (1.41×103 kg/m3)
    = 40.3 · (1.41×103 kg/m3)
    = 5.68×104 kg/m3

    は太陽の密度を表す。以下も参照。

    • Munsell, Kirk (2008年6月11日). “Sun: facts & figures”. Solar system exploration. NASA. 2016年8月26日

    interstellar.jpl.nasa.gov

    jpl.nasa.gov

    nasa.gov

    nssdc.gsfc.nasa.gov

    • Williams, D. R. (2006年2月10日). “Moon fact sheet”. NASA. 2016年8月28日閲覧。

nature.com

nazology.net

nhk.or.jp

www3.nhk.or.jp

nih.gov

pubmed.ncbi.nlm.nih.gov

ncbi.nlm.nih.gov

pmc.ncbi.nlm.nih.gov

nytimes.com

reference.com

dictionary.reference.com

rochester.edu

pas.rochester.edu

saao.ac.za

sciencedaily.com

sciencemag.org

advances.sciencemag.org

scientificamerican.com

space.com

telegraph.co.uk

u-strasbg.fr

simbad.u-strasbg.fr

unam.mx

astroscu.unam.mx

  • Adams, Fred C.; Laughlin, Gregory; Graves, Genevieve J. M (2004). Red dwarfs and the end of the main sequence (PDF). Gravitational collapse: from massive stars to planets. Vol. 22. Revista Mexicana de Astronomía y Astrofísica. pp. 46–49.

unistra.fr

vizier.cds.unistra.fr

unizar.es

zaguan.unizar.es

utexas.edu

clyde.as.utexas.edu

web.archive.org

worldcat.org

search.worldcat.org