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pro vyhledávání: '"Tayar, Jamie N."'
Autor:
Avallone, Ellis A., Tayar, Jamie N., van Saders, Jennifer L., Berger, Travis A., Claytor, Zachary R., Beaton, Rachael L., Teske, Johanna, Godoy-Rivera, Diego, Pan, Kaike
Stellar rotation is a complex function of mass, metallicity, and age and can be altered by binarity. To understand the importance of these parameters in main sequence stars, we have assembled a sample of observations that spans a range of these param
Externí odkaz:
http://arxiv.org/abs/2203.15116