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Titlebook: Uncertainty Management with Fuzzy and Rough Sets; Recent Advances and Rafael Bello,Rafael Falcon,José Luis Verdegay Book 2019 Springer Nat

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Juan Carlos Figueroa-García,Eduyn-Ramiro López-Santana,Germán-Jairo Hernández-Pérezhood. The brightness of HII regions allows them to be a useful tool in estimating the star formation rate in distant galaxies. The UV radiation from massive stars can have a significant effect on the evaporation of protostellar disks around lower-mass stars in the same cluster.
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Flabio Gutierrez,Edwar Lujan,Rafael Asmat,Edmundo Vergaras just like a regularMendelian locus. For small-effect QTL, we simply cannot observe the segregation and must resort to statistical methods to infer the segregation. Most statistical methods applied in quantitative genetics require specific genetic models, which will be the focus of this chapter.
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Daryl H. Hepting,Hadeel Hatim Bin Amer,Yiyu Yaong a function of all the variables involved (the values of all the variables at each instant). Therefore, the position of the “image point” representing the state of the system will be, at some point within the space, continuously moving as time advances, following the minute changes of the variables’ values.
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