Hertzsprungi-Russelli diagramm (Estonian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Hertzsprungi-Russelli diagramm" in Estonian language version.

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aavso.org

Gingerich, Owen (2013). "The Critical Importance of Russell's Diagram".
Crowther, P. A., Schnurr, O., Hirschi, R., Yusof, N., Parker, R. J., Goodwin, S. P. ja Kassim, A. H. (2010). "The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit".{{netiviide}}: CS1 hooldus: mitu nime: autorite loend (link)
Banerjee, S., Kroupa, P. ja Oh S. (2012). "The emergence of super-canonical stars in R136-type star-burst clusters".{{netiviide}}: CS1 hooldus: mitu nime: autorite loend (link)
Ohkubo, T., Nomoto, K., Umeda, H., Yoshida, N. ja Tsuruta, S. (2009). "Evolution of Very Massive Population III Stars with Mass Accretion from Pre-Main Sequence to Collapse".{{netiviide}}: CS1 hooldus: mitu nime: autorite loend (link)

Laughlin, G., Bodenheimer, P. ja Adams, F. C. (1996). "The End of the Main Sequence".{{netiviide}}: CS1 hooldus: mitu nime: autorite loend (link)

Carme, J. ja Masana, E. (2008). "The Physical Characterization of the Stars" (PDF).{{netiviide}}: CS1 hooldus: mitu nime: autorite loend (link)