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- W2755042971 abstract "Small volume statistics show, that luminosity of slow rotating stars is proportional to their angular momentums of rotation. Cause should be outside of standard solar model. Slow rotating giants and dim dwarfs are not out of „main sequence” in this concept. Predictive power of stellar mass-radius- equatorial rotation speed-luminosity relation has been offered to test in numerous examples." @default.
- W2755042971 created "2017-09-25" @default.
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- W2755042971 date "2017-09-01" @default.
- W2755042971 modified "2023-09-23" @default.
- W2755042971 title "Basics of Astrophysics Revisited. I. Mass Luminosity Relation for K, M and G Class Stars" @default.
- W2755042971 hasPublicationYear "2017" @default.
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