Unusual Isotopic Abundances in a Fully Convective Stellar Binary

Unusual Isotopic Abundances in a Fully Convective Stellar Binary

Low-mass M dwarfs represent the most common outcome of star formation, but their complex emergent spectra hinder detailed studies of their composition and initial formation. The measurement of isotopic ratios is a key tool that has been used to unlock the formation of our solar system, the Sun, and...

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Bibliographic Details
Main Authors: Lothringer, J. D., Flores, B., Mills, E. A. C., Freedman, R., Valverde, J., Miles, B., Skemer, A., Crossfield, Ian Jm, Guo, Xueying
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Published: American Astronomical Society/IOP Publishing 2019
Online Access:https://hdl.handle.net/1721.1/121390

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https://hdl.handle.net/1721.1/121390

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