Andromeda tumanligi (Uzbek Wikipedia)

Analysis of information sources in references of the Wikipedia article "Andromeda tumanligi" in Uzbek language version.

refsWebsite

Global rank Uzbek rank

2^nd place

3^rd place

5,591^st place

9,522^nd place

5^th place

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26^th place

78^th place

aanda.org

López-Corredoira, M.; Prieto, C. Allende; Garzón, F.; Wang, H.; Liu, C.; Deng, L. (1 April 2018). "Disk stars in the Milky Way detected beyond 25 kpc from its center". Astronomy & Astrophysics 612: L8. doi:10.1051/0004-6361/201832880. ISSN 0004-6361. https://www.aanda.org/articles/aa/abs/2018/04/aa32880-18/aa32880-18.html.

doi.org

dx.doi.org

López-Corredoira, M.; Prieto, C. Allende; Garzón, F.; Wang, H.; Liu, C.; Deng, L. (1 April 2018). "Disk stars in the Milky Way detected beyond 25 kpc from its center". Astronomy & Astrophysics 612: L8. doi:10.1051/0004-6361/201832880. ISSN 0004-6361. https://www.aanda.org/articles/aa/abs/2018/04/aa32880-18/aa32880-18.html.
Payne-Gaposchkin, Cecilia H. (1953). "Why Do Galaxies Have a Spiral Form?". Scientific American 189 (3): 89–99. doi:10.1038/scientificamerican0953-89. http://www.jstor.org/stable/24944338.

jstor.org

Payne-Gaposchkin, Cecilia H. (1953). "Why Do Galaxies Have a Spiral Form?". Scientific American 189 (3): 89–99. doi:10.1038/scientificamerican0953-89. http://www.jstor.org/stable/24944338.

worldcat.org

López-Corredoira, M.; Prieto, C. Allende; Garzón, F.; Wang, H.; Liu, C.; Deng, L. (1 April 2018). "Disk stars in the Milky Way detected beyond 25 kpc from its center". Astronomy & Astrophysics 612: L8. doi:10.1051/0004-6361/201832880. ISSN 0004-6361. https://www.aanda.org/articles/aa/abs/2018/04/aa32880-18/aa32880-18.html.