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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Main Authors: Lothringer, J. D. (Author), Flores, B. (Author), Mills, E. A. C. (Author), Freedman, R. (Author), Valverde, J. (Author), Miles, B. (Author), Skemer, A. (Author), Crossfield, Ian Jm (Author), Guo, Xueying (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: American Astronomical Society/IOP Publishing, 2019-06-24T14:47:03Z.
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