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Ypsilon Pegasi (Polish Wikipedia)

Analysis of information sources in references of the Wikipedia article "Ypsilon Pegasi" in Polish language version.

refsWebsite
Global rank Polish rank
3doi.org
2nd place
6th place
2harvard.edu
18th place
140th place
2u-strasbg.fr
1,342nd place
566th place
1semanticscholar.org
11th place
1,348th place
1worldcat.org
5th place
2nd place
1uchicago.edu
230th place
435th place
1iau.org
1,985th place
942nd place

doi.org

doi.org

  • R.O. Gray, M.G. Napier, L.I. Winkler. The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars. „Astronomical Journal”. 121 (4), s. 2148–2158, 2001. DOI: 10.1086/319956. Bibcode: 2001AJ....121.2148G. 
  • R.O. Gray, P.W. Graham, S.R. Hoyt. The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. II. Basic Parameters of Program Stars and the Role of Microturbulence. „Astronomical Journal”. 121 (4), s. 2159–2172, 2001. DOI: 10.1086/319957. Bibcode: 2001AJ....121.2159G. 

dx.doi.org

harvard.edu

adsabs.harvard.edu

  • R.O. Gray, M.G. Napier, L.I. Winkler. The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars. „Astronomical Journal”. 121 (4), s. 2148–2158, 2001. DOI: 10.1086/319956. Bibcode: 2001AJ....121.2148G. 
  • R.O. Gray, P.W. Graham, S.R. Hoyt. The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. II. Basic Parameters of Program Stars and the Role of Microturbulence. „Astronomical Journal”. 121 (4), s. 2159–2172, 2001. DOI: 10.1086/319957. Bibcode: 2001AJ....121.2159G. 

iau.org

  • Naming Stars. Międzynarodowa Unia Astronomiczna, 2018-08-10. [dostęp 2018-12-05].

semanticscholar.org

u-strasbg.fr

simbad.u-strasbg.fr

vizier.u-strasbg.fr

uchicago.edu

penelope.uchicago.edu

worldcat.org