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New Binary System of Brown Dwarfs Exhibits Stable Mass Transfer
Astronomers have identified a binary system of brown dwarfs, ZTF J1239+8347, which demonstrates stable mass transfer between its components. This discovery has implications for our understanding of brown dwarf interactions.
Editorial Staff
1 min read
The recent discovery of the binary system ZTF J1239+8347, made by astronomers from Caltech and other institutions, highlights a significant interaction between two brown dwarfs.
This system is characterized by stable mass transfer, a phenomenon that can affect the evolution and characteristics of both brown dwarfs involved.
Understanding such binary systems is crucial for advancing knowledge of stellar formation and the lifecycle of substellar objects.