NGC 2420 (Czech Wikipedia)

Analysis of information sources in references of the Wikipedia article "NGC 2420" in Czech language version.

refsWebsite

Global rank Czech rank

8harvard.edu

18^th place

99^th place

2arxiv.org

69^th place

196^th place

2doi.org

2^nd place

4^th place

1web.archive.org

1^st place

1u-strasbg.fr

1,342^nd place

1,190^th place

1cseligman.com

low place

1wz.cz

low place

135^th place

arxiv.org (Global: 69^th place; Czech: 196^th place)

DIAS, W. S.; ALESSI, B. S.; MOITINHO, A., et al. New catalogue of optically visible open clusters and candidates. S. 871–873. Astronomy and Astrophysics [online]. Červenec 2002 [cit. 2021-01-13]. Roč. 389, s. 871–873. Dostupné online. arXiv astro-ph/0203351. doi:10.1051/0004-6361:20020668. Bibcode 2002A&A...389..871D. (anglicky)
SEMENOVA, Ekaterina; BERGEMANN, Maria; DEAL, Morgan, et al. The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations. S. 15. Astronomy and Astrophysics [online]. Listopad 2020 [cit. 2021-01-13]. Roč. 643, s. 15. Dostupné online. arXiv 2007.09153. doi:10.1051/0004-6361/202038833. Bibcode 2020A&A...643A.164S. (anglicky)

cseligman.com (Global: low place; Czech: low place)

SELIGMAN, Courtney. Celestial Atlas: NGC 2420 (= OCL 488) [online]. [cit. 2021-01-13]. Dostupné online. (anglicky)

doi.org (Global: 2^nd place; Czech: 4^th place)

DIAS, W. S.; ALESSI, B. S.; MOITINHO, A., et al. New catalogue of optically visible open clusters and candidates. S. 871–873. Astronomy and Astrophysics [online]. Červenec 2002 [cit. 2021-01-13]. Roč. 389, s. 871–873. Dostupné online. arXiv astro-ph/0203351. doi:10.1051/0004-6361:20020668. Bibcode 2002A&A...389..871D. (anglicky)
SEMENOVA, Ekaterina; BERGEMANN, Maria; DEAL, Morgan, et al. The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations. S. 15. Astronomy and Astrophysics [online]. Listopad 2020 [cit. 2021-01-13]. Roč. 643, s. 15. Dostupné online. arXiv 2007.09153. doi:10.1051/0004-6361/202038833. Bibcode 2020A&A...643A.164S. (anglicky)

harvard.edu (Global: 18^th place; Czech: 99^th place)

ui.adsabs.harvard.edu

DIAS, W. S.; ALESSI, B. S.; MOITINHO, A., et al. New catalogue of optically visible open clusters and candidates. S. 871–873. Astronomy and Astrophysics [online]. Červenec 2002 [cit. 2021-01-13]. Roč. 389, s. 871–873. Dostupné online. arXiv astro-ph/0203351. doi:10.1051/0004-6361:20020668. Bibcode 2002A&A...389..871D. (anglicky)
COLLINDER, Per. On Structural Properties of Open Galactic Clusters and their Spatial Distribution. Catalog of Open Galactic Clusters. S. B1-B46. Annals of the Observatory of Lund [online]. 1931 [cit. 2021-01-13]. Čís. 2, s. B1-B46. Dostupné online. Bibcode 1931AnLun...2....1C. (anglicky)
MELOTTE, P. J. A Catalogue of Star Clusters shown on Franklin-Adams Chart Plates. S. 175. Memoirs of the Royal Astronomical Society [online]. 1915 [cit. 2021-01-13]. Roč. 60, s. 175. Dostupné online. Bibcode 1915MmRAS..60..175M. (anglicky)
SEMENOVA, Ekaterina; BERGEMANN, Maria; DEAL, Morgan, et al. The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations. S. 15. Astronomy and Astrophysics [online]. Listopad 2020 [cit. 2021-01-13]. Roč. 643, s. 15. Dostupné online. arXiv 2007.09153. doi:10.1051/0004-6361/202038833. Bibcode 2020A&A...643A.164S. (anglicky)

adsabs.harvard.edu

DIAS, W. S.; ALESSI, B. S.; MOITINHO, A., et al. New catalogue of optically visible open clusters and candidates. S. 871–873. Astronomy and Astrophysics [online]. Červenec 2002 [cit. 2021-01-13]. Roč. 389, s. 871–873. Dostupné online. arXiv astro-ph/0203351. doi:10.1051/0004-6361:20020668. Bibcode 2002A&A...389..871D. (anglicky)
COLLINDER, Per. On Structural Properties of Open Galactic Clusters and their Spatial Distribution. Catalog of Open Galactic Clusters. S. B1-B46. Annals of the Observatory of Lund [online]. 1931 [cit. 2021-01-13]. Čís. 2, s. B1-B46. Dostupné online. Bibcode 1931AnLun...2....1C. (anglicky)
MELOTTE, P. J. A Catalogue of Star Clusters shown on Franklin-Adams Chart Plates. S. 175. Memoirs of the Royal Astronomical Society [online]. 1915 [cit. 2021-01-13]. Roč. 60, s. 175. Dostupné online. Bibcode 1915MmRAS..60..175M. (anglicky)
SEMENOVA, Ekaterina; BERGEMANN, Maria; DEAL, Morgan, et al. The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations. S. 15. Astronomy and Astrophysics [online]. Listopad 2020 [cit. 2021-01-13]. Roč. 643, s. 15. Dostupné online. arXiv 2007.09153. doi:10.1051/0004-6361/202038833. Bibcode 2020A&A...643A.164S. (anglicky)

u-strasbg.fr (Global: 1,342^nd place; Czech: 1,190^th place)

simbad.u-strasbg.fr

SIMBAD Astronomical Database: Results for NGC 2420 [online]. [cit. 2021-01-13]. Dostupné online. (anglicky)

web.archive.org (Global: 1^st place; Czech: 1^st place)

FROMMERT, Hartmut. Revised NGC Data for NGC 2420 [online]. SEDS.org [cit. 2021-01-13]. Dostupné v archivu pořízeném dne 2020-10-28. (anglicky)

wz.cz (Global: low place; Czech: 135^th place)

hvezdnouoblohou.wz.cz

KODRIŠ, Michal. Průvodce hvězdnou oblohou: Blizenci [online]. [cit. 2021-01-13]. Dostupné online.

NGC 2420 (Czech Wikipedia)

arxiv.org (Global: 69th place; Czech: 196th place)

cseligman.com (Global: low place; Czech: low place)

doi.org (Global: 2nd place; Czech: 4th place)

harvard.edu (Global: 18th place; Czech: 99th place)